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Star in the constellation Cygnus
Lambda Cygni (λ Cyg) is a class B5V (blue main-sequence) star in the constellation Cygnus. Its apparent magnitude is 4.54 and it is approximately 770 light
Lambda_Cygni
Star in the constellation Cygnus
8 Andromedae, Lambda Andromedae, Kappa Andromedae, Psi Andromedae and Iota Andromedae. Consequently, the Chinese name for Pi1 Cygni itself is 螣蛇四 (Téng
Pi1_Cygni
A-type main sequence star in the constellation Cygnus
29 Cygni (also widely known as HIP 99770) is a single star in the northern constellation of Cygnus. It is dimly visible to the naked eye as a white-hued
29_Cygni
Type of star that is luminous, blue, and variable in brightness
one of the brightest stars of the Large Magellanic Cloud. The LBV stars P Cygni and η Carinae have been known as unusual variables since the 17th century
Luminous_blue_variable
Pattern of stars recognized on Earth's night sky
simple geometric shapes. The Summer Triangle of Deneb, Altair, and Vega – α Cygni, α Aquilae, and α Lyrae – is prominent in the northern hemisphere summer
Asterism_(astronomy)
Binary star system in the constellation of Andromeda
an asterism consisting of λ Andromedae, α Lacertae, 4 Lacertae, π2 Cygni, π1 Cygni, HD 206267, ε Cephei, β Lacertae, σ Cassiopeiae, ρ Cassiopeiae, τ Cassiopeiae
Lambda_Andromedae
Visible star that is nearly aligned with Earth's axis of rotation
close enough to be taken as marking the pole, while third-magnitude Delta Cygni will be a more helpful pole star, at a distance of 3° from celestial north
Pole_star
Hot, luminous star with a spectral type of A9 or earlier
Wolf Rayet star.[citation needed] Many blue supergiant stars are Alpha Cygni variables. While the stellar wind from a red supergiant is dense and slow
Blue_supergiant
Stars with a supergiant luminosity class with a spectral type of K or M
examples: Antares A Betelgeuse Epsilon Pegasi Zeta Cephei Lambda Velorum Eta Persei 31 and 32 Cygni Psi1 Aurigae 119 Tauri Mira was historically thought to
Red_supergiant
Rare star with tremendous luminosity and high rates of mass loss by stellar winds
overall NML Cygni S Persei VY Canis Majoris - potentially the largest star known in the Milky Way VX Sagittarii KY Cygni BC Cygni BI Cygni RW Cygni NR Vulpeculae
Hypergiant
Constellation in the southern celestial hemisphere
all visible to the unaided eye, as ranks behind Groombridge 1830 and 61 Cygni, and the ninth-highest overall. This will move the star into Tucana around
Indus_(constellation)
Denebola Star 2.17 Gamma Centauri Binary star system 2.21 2.14 Lambda Velorum Star 2.23 Gamma Cygni Star Suspected variable star 2.23 Alpha Cassiopeiae Star
List of brightest natural objects in the sky
List_of_brightest_natural_objects_in_the_sky
Motto of the City of Westminster custos morum keeper of morals A censor cygnis insignis distinguished by its swans Motto of Western Australia cygnus inter
List_of_Latin_phrases_(full)
Light from the stars
7 × 10 − 3 {\displaystyle q=7\times 10^{-3}} for the red supergiant NML Cygni and q = 2 × 10 − 3 {\displaystyle q=2\times 10^{-3}} in the long-period
Starlight
Hypothetical compact star
hole. Some stellar black holes might be grey holes, two of which are V404 Cygni and Cygnus X-1. Q-ball B-ball, stable Q-balls with a large baryon number
Q_star
Stellar classification
unchanged over the years, are: Sigma Draconis (K0 V) Epsilon Eridani (K2 V) 61 Cygni A (K5 V) Other primary MK standard stars include: 70 Ophiuchi A (K0 V),
K-type_main-sequence_star
Fomalhaut α Piscis Austrini 0025 A3 V Southern 19 1.25 (1.21–1.29var) Deneb α Cygni 2,600 A2 Ia Northern 20 1.25 (1.23–1.31var) Mimosa β Crucis 0280 B0.5 III
List_of_brightest_stars
originally from Arabic: البالع al-bāliʿ ('the swallower'). /ælˈbeɪli/ Albireo β1 Cygni Aa Cygnus unknown The source of the name Albireo is not entirely clear.
List_of_proper_names_of_stars
1 (or Icarus) — second most distant star, 9 billion light years away. P Cygni — suddenly brightened in the 17th century WNC4 — Messier Object 40 Zeta
Lists_of_stars
Star whose brightness fluctuates, as seen from Earth
later named Mira, was discovered in the 17th century, followed by Chi Cygni then R Hydrae. By 1786, ten had been documented. Variable star discovery
Variable_star
Stellar classification
Majoris (G8V). Other primary MK standard stars include HD 115043 (G1V) and 16 Cygni B (G3V). The choices of G4 and G6 dwarf standards have changed slightly
G-type_main-sequence_star
Multiple star system in the constellation Sagittarius
96). In addition, it shows more irregular variations typical of an Alpha Cygni variable, irregularly pulsating hot supergiant stars. Mu Sagittarii A appears
Mu_Sagittarii
60 ±0.9 A & B flare stars B M? 0.11 13.27 15.58 C M? 0.10 14.03 16.34 61 Cygni A (BD+38°4343)$ 11.4039 ±0.0012 Cyg* 21h 06m 53.9s +38° 44′ 58″ K5.0V 0
List_of_nearest_stars
Constellation in the southern celestial hemisphere
times and diameter around 80 times that of the Sun. Classified as an Alpha Cygni type variable star, Aludra varies in brightness from magnitude 2.38 to 2
Canis_Major
Crucis 364 ± 9 Crux B5Vne 5.19 Albireo (Beta¹ Cygni) Aa 364.8+15.6 −15.3 Cygnus K2II 3.21 + 5.85 Ab B8:p Lambda Aquarii (Hydor) 365 ± 10 Aquarius M2.5 IIIa
List of star systems within 350–400 light-years
List_of_star_systems_within_350–400_light-years
Classification of stars based on spectral properties
spectral type to indicate peculiar features of the spectrum. For example, 59 Cygni is listed as spectral type B1.5Vnne, indicating a spectrum with the general
Stellar_classification
Constellation in the northern celestial hemisphere
spectrograms - XIX. The superficially normal B stars ζ Draconis, η Lyrae, 8 Cygni and 22 Cygni". Monthly Notices of the Royal Astronomical Society. 296 (4): 856–862
Lyra
Type of variable star
Rapidly oscillating Ap SX Phoenicis Blue-white with early spectra Alpha Cygni Beta Cephei Slowly pulsating B-type PV Telescopii Blue large-amplitude pulsator
Rapidly_oscillating_Ap_star
Observatory Circular. 8: 59–67. Bibcode:1984SAAOC...8...59C. "eSky: 61 Cygni". www.glyphweb.com. Retrieved 2024-01-05. Kervella, Pierre; Mérand, Antoine;
List of nearest stars by spectral type
List_of_nearest_stars_by_spectral_type
Brightest star in the constellation Lyra
and, when Bessel published a parallax of 0.314″ for the star system 61 Cygni, Struve revised his value for Vega's parallax to nearly double the original
Vega
Star system in the Centaurus constellation
1839 after Bessel released his own accurately determined parallax for 61 Cygni in 1838. For this reason, Alpha Centauri is sometimes considered as the
Alpha_Centauri
Changed position of star vs background
parallax measurements in 1832–1838, for the stars Alpha Centauri, Vega, and 61 Cygni. Stellar parallax is so small that it was unobservable until the 19th century
Stellar_parallax
Type of star that is massive and luminous
of expelled circumstellar materials, which can produce emission lines, P Cygni profiles, or forbidden lines. The MK system assigns stars to luminosity
Supergiant
confirmed exoplanet (KOBE-1b & c). 27 Cygni 78.1 ± 0.2 Cygnus 20h 06m 21.76743s +35° 58′ 20.8875″ G8.5IVa 5.38 Lambda Sagittarii (Kaus Borealis)$ 78.2 Sagittarius
List of star systems within 75–80 light-years
List_of_star_systems_within_75–80_light-years
Variable star in the constellation Orion
this variable was considered unique, but in 1970 a similar star, V1057 Cygni, was discovered, and a number of additional examples have been discovered
FU_Orionis
Beta Capricorni Deneb Dhanab ud-Dajājah Tail of the hen ذنب الدجاجة Alpha Cygni Deneb Algedi Dhanab ul-Jady Tail of the goat ذنب الجدي Delta Capricorni
List_of_Arabic_star_names
Lyrae) Star (part of a double star pair) 1839−1847 7.77 pc (125 mas) 61 Cygni Binary star 1838−1839 3.48 pc (313.6 mas) This was the first star other
List_of_most_distant_stars
Mysterious nearly periodic radial velocity variations in the eccentric binary ε Cygni", Astronomy & Astrophysics, 647: A160, arXiv:2102.01999, Bibcode:2021A&A
List_of_nearest_giant_stars
intensity interferometry to determine the distances of the blue supergiants P Cygni and Rigel". Monthly Notices of the Royal Astronomical Society. 515 (1):
List_of_supernova_candidates
Constellation in the northern celestial hemisphere
(2012). "A new interferometric study of four exoplanet host stars : θ Cygni, 14 Andromedae, υ Andromedae and 42 Draconis". Astronomy & Astrophysics
Andromeda_(constellation)
Brunthaler, A. (2012). "The distance and size of the red hypergiant NML Cygni from VLBA and VLA astrometry". Astronomy & Astrophysics. 544: A42. arXiv:1207
List_of_largest_stars
Class of young variable stars
around a K-type star PDS 70b around a K-type star Orion variable EX Lupi P Cygni profile Appenzeller, I; Mundt, R (1989). "T Tauri stars". The Astronomy
T_Tauri_star
Symbiotic nova in the constellation of Sagitta
R. C.; et al. (July 1978), "Infrared spectra of HM Sagittae and V1016 Cygni", Astrophysical Journal, 223: L93–L95, Bibcode:1978ApJ...223L..93P, doi:10
HM_Sagittae
5IVp 5.02 Mintaka Aa1 (Delta Orionis) 1,200 3 O9.5II 2.5 V2119 Cygni 1203±22.3 1 sdO 60 Cygni 1225±57 1 sdO Upsilon Orionis 1,260±75 1 B0V or O9.7V +4.618±0
List_of_O-type_stars
Type of large cool star
Aurigae) Schedar (α Cassiopeiae) δ Andromedae ρ Persei Mira (ο Ceti) χ Cygni Rasalgethi (α Herculis) The Sun will exit the main sequence in approximately
Red_giant
Type of cool giant star
with a hotter companion which may also be variable. The Mira variable Chi Cygni is an intrinsic S star. When near maximum light, it is the sky's brightest
S-type_star
Continuous band of stars that appears on plots of stellar color versus brightness
78 000,000.40 05,240 70 Ophiuchi A K5 00.74 000.69 000,000.16 04,410 61 Cygni A M0 00.51 000.60 000,000.072 03,800 Lacaille 8760 M5 00.18 000.15 000,000
Main_sequence
Systematic designations to unambiguously identify astronomical objects
designations mark them as variable stars. Examples include R Cygni, RR Lyrae, and V1331 Cygni. The International Astronomical Union delegates the task to
Astronomical naming conventions
Astronomical_naming_conventions
Large self-illuminated object in space
early 1900s. The first direct measurement of the distance to a star (61 Cygni at 11.4 light-years) was made in 1838 by Friedrich Bessel using the parallax
Star
Clandestine term
Toliman (Alpha Centauri), Kuma (Nu Draconis), Deneb (Alpha Cygni), Propus (Eta Geminorum), Heka (Lambda Orionis), Rana (Delta Eridani), Regor (Gamma Velorum)
Code_name
Constellation in the northern celestial hemisphere
of calcium and hydrogen. Its spectral type is G5V:e. SS Aurigae is an SS Cygni-type variable star, classified as an explosive dwarf. Discovered by Emil
Auriga
Stellar explosions that appear to be supernovae
examples of supernova impostors include the Great Eruption of Eta Carinae, P Cygni, SN 1961V, SN 1954J, SN 1997bs, SN 2008S, and SN 2010dn where detections
Supernova_impostor
Feature of the Hertzsprung-Russell diagram
gap include: Epsilon Pegasi Pi Puppis Epsilon Geminorum Beta Arae Gamma Cygni Capella B Canopus, Iota Carinae, and Upsilon Carinae are also starting to
Hertzsprung_gap
Star group in the constellation Cygnus
Another prominent member of the cluster is the eclipsing binary star V470 Cygni [mk] (HD 228911). The cluster lies at a distance of about 3500 light years
HD_193322
Stage of stellar evolution
being a red supergiant. Extreme red hypergiants VY Canis Majoris and NML Cygni are two such known candidates for a star within a second red supergiant
Blue_loop
1337s −12° 57′ 21.924″ M7.5 B M7.5 C L7.0 WISE 1717+6129 72.7 T8 Epsilon Cygni (Aljanah) 72.7 ± 0.2 Cygnus 20h 46m 12.68236s +33° 58′ 12.9250″ K0III 2
List of star systems within 70–75 light-years
List_of_star_systems_within_70–75_light-years
List from the Alphabet Direction (αβ)
clusters) (for example: Turner 9 at and near the variable star SU Cygni, aka 'SU Cygni cluster') UBV — Photoelectric Catalogue, magnitude and color of stars
List of astronomical catalogues
List_of_astronomical_catalogues
Type of star, larger and brighter than the Sun
giant. Mira (ο Ceti), an M-type giant and prototype Mira variable. Chi Cygni, a S-type giant. TX Piscium, a C-type giant (carbon star). Giant stars with
Giant_star
Heterogeneous class of stars with unusual spectra
Wolf–Rayet emission lines frequently have a broadened absorption wing (P Cygni profile) suggesting circumstellar material. A WO sequence has also been
Wolf–Rayet_star
Methods for estimating the age of a star
like VY Canis Majoris, one of the largest stars known, together with NML Cygni, VX Sagittarii and Trumpler 27-1 all have radii larger than that of the
Stellar_age_estimation
Sun-centered astronomical model
than zero by measuring the parallax of 0.314 arcseconds of a star named 61 Cygni. In the same year Friedrich Georg Wilhelm Struve and Thomas Henderson measured
Heliocentrism
Precession of a gyroscope due to a nearby celestial body's rotation affecting spacetime
a change was observed in 2019 with the black hole X-ray binary in V404 Cygni. Pulsars emit rapidly repeating radio pulses with extremely high regularity
Lense–Thirring_precession
Region of an astronomical diagram
high luminosity supergiants are somewhat variable, including the Alpha Cygni variables. In the specific region of more luminous stars above the instability
Instability_strip
Lyrae) Star (part of a double star pair) 1839–1847 7.77 pc (125 mas) 61 Cygni Binary star 1838−1839 3.48 pc (313.6 mas) This was the first star other
List of the most distant astronomical objects
List_of_the_most_distant_astronomical_objects
Holes, astronomer Phil Charles; the Japanese Ginga (satellite) and V404 Cygni, which orbits a black hole; the William Herschel Telescope in La Palma;
List_of_Equinox_episodes
Slow irregular eruptive variable stars
white dwarf after its outburst. One example of a symbiotic nova is V1016 Cygni, whose outburst in 1971–2007 clearly indicated a thermonuclear explosion
Symbiotic_nova
Aries K2 III 4.349 Theta Leonis (Chertan) 165 ± 1 Leo A2 V 3.324 Delta Cygni (Fawaris) 165 ± 4 Cygnus A0 IV 2.87 BD−22 5866 A 166 K7 10.1 B K7 C M1 D
List of star systems within 150–200 light-years
List_of_star_systems_within_150–200_light-years
Brightness of a celestial object observed from the Earth
seen from 1 AU away −39.66 star R136a1 seen from 1 AU away −39.47 star P Cygni seen from 1 AU away −38.00 star Rigel seen from 1 AU away would be seen
Apparent_magnitude
System of two stars orbiting each other
binaries include 61 Cygni (a binary in the constellation Cygnus, composed of two K class (orange) main-sequence stars, 61 Cygni A and 61 Cygni B, which is known
Binary_star
intensity interferometry to determine the distances of the blue supergiants P Cygni and Rigel". Monthly Notices of the Royal Astronomical Society. 515 (1):
List_of_nearest_supergiants
Constellation split into two non-contiguous parts
89 and 7.07 in 87 days. This star has been found to display an inverse P Cygni profile, where cold infalling gas on to the star creates redshifted hydrogen
Serpens
List of largest planets by size
(December 2011). "Spectroscopy of very low mass stars and brown dwarfs in the Lambda Orionis star forming region. I. Enlarging the census down to the planetary
List_of_largest_exoplanets
−16° 42′ 58.0″ 8.60 ε Eridani K2V 3.72 6.18 03h 32m 55.84s −09° 27′ 29.7″ 10.5 61 Cygni A K5.0V 5.20 7.49 21h 06m 53.94s +38° 44′ 57.9″ 11.4 B K7.0V 6.05 8.33 Procyon
List_of_nearest_bright_stars
Open cluster in the constellation Cepheus
have been companions of those stars. It has been suggested that Lambda Cephei and 68 Cygni are runaway stars from that area. The core radius of the cluster
NGC_7160
Process by which stars are named
letters. Such designations mark them as variable stars. Examples include R Cygni, RR Lyrae, and GN Andromedae. (Many variable stars also have designations
Stellar designations and names
Stellar_designations_and_names
Overview of the scientific field of astronomy
Semiregular variable Slow irregular variable Other RV Tauri variable Alpha Cygni variable Pulsating white dwarf Eruptive Pre-main sequence star Herbig Ae/Be
Outline_of_astronomy
Set of non-stellar objects in orbit around a star
display much higher orbital eccentricity. An example of such a system is 16 Cygni. The mutual inclination between two planets is the angle between their orbital
Planetary_system
V346 Puppis 1,875 C Leo A 22 1,900 C 2,600,000 S Aurigae 1,940 C-N5+ V1426 Cygni 1,975 C7,2e Sextans A 20 2,000 C 4,310,000 Leo A 226 2,000 C 2,600,000 Sextans
List_of_coolest_stars
Star types predicted by theory
exotic state of matter where most light does not escape the star. V404 Cygni Quark star Star composed of quark matter or strange matter. 3C 58, PSR B0943+10
Hypothetical_star
de Souza, A.; Fouché, M.; et al. (2020). "Intensity interferometry of P Cygni in the H α emission line: Towards distance calibration of LBV supergiant
List_of_most_massive_stars
doi:10.1093/mnras/4.19.168. Bessel, F. W. (1838b). "On the parallax of 61 Cygni". Monthly Notices of the Royal Astronomical Society. 4 (17): 152–161. Bibcode:1838MNRAS
Timeline of cosmological theories
Timeline_of_cosmological_theories
Exoplanets confirmed or discovered from direct imaging
Bouy H (1 June 2007). "The young, wide and very low mass visual binary Lambda Orionis 167". Astronomy and Astrophysics. 468 (1): L5–L8. arXiv:0704.2469
List of directly imaged exoplanets
List_of_directly_imaged_exoplanets
Measure of observed changes in the apparent locations of stars
naked eye (conservatively limiting unaided visual magnitude to 6.0), 61 Cygni A (magnitude V=5.20) has the highest proper motion at 5.281″ yr−1, discounting
Proper_motion
to the Sun. He also discovered the proper motion of the double star 61 Cygni. The asteroid 1000 Piazzia and a Moon's crater have been christened with
List of Italian inventions and discoveries
List_of_Italian_inventions_and_discoveries
intensity interferometry to determine the distances of the blue supergiants P Cygni and Rigel". Monthly Notices of the Royal Astronomical Society. 515 (1):
List_of_star_extremes
Herbig Ae star in the constellation Sagittarius
163296 is a Herbig Ae star due to the H-alpha and NaD lines having a P Cygni profile. The status as a Herbig Ae star was questioned at the time. It was
HD_163296
Stars that host planetary systems
Kepler-16b). A few dozen planets in triple star systems are known (e.g. 16 Cygni Bb) and one in quadruple systems Kepler 64. The Kepler results indicate
Planet-hosting_star
Stars sorted by absolute magnitude
Vernet, D.; Kaiser, R.; Guerin, W. (2020). "Intensity interferometry of P Cygni in the H α emission line: Towards distance calibration of LBV supergiant
List_of_most_luminous_stars
Type of variable star
stars where the spectral type or luminosity is unclear. The K5 star CO Cygni is given as a representative example. Irregular variable supergiants of
Slow_irregular_variable
Stars that have properties between Asymptotic Giant Branch stars and red supergiants
similar stage in life to red giant stars, such as Aldebaran, Mira, and Chi Cygni, and are at a stage where they start to brighten, and their brightness tends
Super-AGB_star
Type of star
Sagittarii VY Canis Majoris AH Scorpii MY Cephei PZ Cassiopeiae IRC −30308 NML Cygni IRC +10420 WOH G64 A IRAS 05280−6910 IRC −10414 RSGC1-F13 CD-34 11794 Although
OH/IR_star
the class ACYG – (celestial object) Alpha CYGni, a class of rotating variable stars named after Alpha Cygni (Deneb), the archetype for the class ADAF
List_of_astronomy_acronyms
Binary star system in the constellation Cassiopeia
Cassiopeiae (Caph), Kappa Cassiopeiae, Alpha Cassiopeiae (Schedar) and Lambda Cassiopeiae. Consequently, the Chinese name for Eta Cassiopeiae itself is
Eta_Cassiopeiae
of the accretion disc and jets 1989 — Identification of microquasar V404 Cygni as a binary black hole candidate system 1989 - Eric Poisson and Werner Israel
Timeline of black hole physics
Timeline_of_black_hole_physics
that Algol's brightness varies 1686 — Gottfried Kirch notices that Chi Cygni's brightness varies 1718 — Edmund Halley discovers stellar proper motions
Timeline_of_stellar_astronomy
Sneppen, Albert; Watson, Darach (July 1, 2023). "Discovery of a 760 nm P Cygni line in AT2017gfo: Identification of yttrium in the kilonova photosphere"
Timeline of gravitational physics and relativity
Timeline_of_gravitational_physics_and_relativity
Star in the constellation Cygnus
runaway stars known in the Milky Way (along with the O-type supergiants Lambda Cephei and Zeta Puppis). Initially it was suggested a supernova explosion
BD+43_3654
LAMBDA CYGNI
LAMBDA CYGNI
Boy/Male
Indian
Jaws.
Girl/Female
Muslim
Soft to touch
Surname or Lastname
English
English : habitational name from Lambden in Berwickshire.
Girl/Female
Indian
Dark lipped
Girl/Female
Indian
Ambitious
Female
Greek
(Λαμία) Greek myth name of an evil spirit who abducts and devours children, LAMIA means "large shark." The name means "vampire" in Latin and "fiend" in Arabic.
Girl/Female
Muslim
Flame
Girl/Female
Arabic, Indian, Muslim, Pashtun, Sanskrit
Flame; Large; Spacious; Tall; Another Name for Durga and Lakshmi
Girl/Female
Muslim
Dark lipped
Girl/Female
Indian
Flame
Girl/Female
Muslim
Praiseworthy, Praiser of Allah
Girl/Female
Muslim
Ambitious
Female
Italian
Italian form of English Amber, AMBRA means "amber."
Female
Native American
Native American Indian name ALAMEDA means "grove of cottonwood."
Female
Spanish
Feminine form of Spanish Amado, AMADA means "beloved."
Girl/Female
Indian
Soft to touch
Surname or Lastname
English
English : from Middle English lamb, a nickname for a meek and inoffensive person, or a metonymic occupational name for a keeper of lambs. See also Lamm.English : from a short form of the personal name Lambert.Irish : reduced Anglicized form of Gaelic Ó Luain (see Lane 3). MacLysaght comments: ‘The form Lamb(e), which results from a more than usually absurd pseudo-translation (uan ‘lamb’), is now much more numerous than O’Loan itself.’Possibly also a translation of French agneau.
Boy/Male
Hindu
Lord Ganesh, The huge bellied Lord
Girl/Female
Indian
Praiseworthy, Praiser of Allah
Surname or Lastname
English
English : from a pet form of Lamb 1 and 2.English : from an Old Norse personal name Lambi, from lamb ‘lamb’.
LAMBDA CYGNI
LAMBDA CYGNI
Boy/Male
Hindu, Indian, Marathi
Clever in Work
Boy/Male
Indian, Sanskrit
King of the Planets
Girl/Female
American, British, English, Greek, Irish
Dweller Near a Hollow; From the Round Hill; Maiden; Seething Pool; Ravine
Boy/Male
Indian
Leader, Chief
Girl/Female
Arabic
Female Leopard
Boy/Male
Tamil
Charioteer
Girl/Female
Gujarati, Hindu, Indian, Kannada, Malayalam, Marathi
Who Loves Friends and Family Members
Male
English
English surname transferred to unisex forename use, TATE means "cheerful."
Boy/Male
Indian
Printing
Girl/Female
American, Christian, Greek, Indian, Swedish
Pure; The Celtic Form of Catherine
LAMBDA CYGNI
LAMBDA CYGNI
LAMBDA CYGNI
LAMBDA CYGNI
LAMBDA CYGNI
pl.
of Lamina
n.
A lamb.
n.
A thin plate or scale; a layer or coat lying over another; -- said of thin plates or platelike substances, as of bone or minerals.
n.
A lamb.
n.
A thin plate or lamina.
a.
Lamed; lame; disabled; impeded.
n.
A lamp or candlestick.
p. pr. & vb. n.
of Lamb
n.
A thin plate or scale; specif., one of the thin, flat processes composing the vane of a feather.
n.
The name of the Greek letter /, /, corresponding with the English letter L, l.
n.
The blade of a leaf; the broad, expanded portion of a petal or sepal of a flower.
n.
Any person who is as innocent or gentle as a lamb.
n.
The lamb's-quarters (Chenopodium album).
a.
Shaped like the Greek letter lambda (/); as, the lambdoid suture between the occipital and parietal bones of the skull.
imp. & p. p.
of Lamb
n.
A viola da gamba.
n.
The point of junction of the sagittal and lambdoid sutures of the skull.
n.
A monster capable of assuming a woman's form, who was said to devour human beings or suck their blood; a vampire; a sorceress; a witch.
pl.
of Lamina
v. i.
To bring forth a lamb or lambs, as sheep.