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Nebula
Sharpless 101 (Sh 2-101) is a H II region emission nebula located in the constellation Cygnus. It is sometimes also called the Tulip Nebula because it
Sh_2-101
Diffuse nebula in Cepheus constellation
Sh 2-132, also known as the Lion Nebula, is a diffuse nebula in Cepheus. It is part of the Cep OB1 Association and located in the Perseus Arm of the galaxy
Sh_2-132
Synthesizer
The Roland SH-101 is an analog synthesizer manufactured by the Roland Corporation between 1982 and 1986. Though it did not achieve significant commercial
Roland_SH-101
Sh 2-129 (also known as the Flying Bat Nebula), is a large emission nebula and H II region located in the constellation Cepheus. It is part of the Cepheus
Sh_2-129
Nebula
Sh 2-112 is a nebula in Cygnus. It is located within the Orion Arm, and is near star complex Cygnus X. It is ionized by the central star BD+45 3216. It
Sh_2-112
Nebula
Sh 2-185 is an H II region centered on the massive star system Gamma Cassiopeiae (γ Cas) in the northern constellation of Cassiopeia. It was included in
Sh_2-185
Emission nebula in Cygnus constellation
Sh 2-114 (also known as Flying Dragon Nebula) is a faint emission nebula located in the constellation of Cygnus. It lies roughly 4° East-Northeast of star
Sh_2-114
Emission nebula in the constellation Orion
Sh 2-279 (alternatively designated S279 or Sharpless 279) is an HII region and bright nebulae that includes a reflection nebula located in the constellation
Sh_2-279
Closest planetary nebulae
Sh 2-216 (also known as Sharpless 216) is an ancient planetary nebula located in the constellation Perseus. It is notable for being the closest planetary
Sh_2-216
Emission nebula or WR* in Canis major
Sh 2-308, also designated as Sharpless 308, RCW 11, or LBN 1052, and commonly known as the Dolphin-Head Nebula, is an H II region located near the center
Sh_2-308
Emission nebula
Sh 2-37, also known by the designation IC 1284, or the common name Twiddlebug Nebula, is an emission nebula in the constellation Sagittarius. It is located
Sh_2-37
Sh 2-115 is an emission nebula and H II region in the constellation of Cygnus, catalogued by Stewart Sharpless in his 1959 second edition of H II regions
Sh_2-115
H II region in the constellation Cepheus
Sh 2-155 (also designated Caldwell 9, Sharpless 155 or S155, or LBN529) is a diffuse nebula in the constellation Cepheus, within a larger nebula complex
Sh_2-155
Planetary nebula
Sh 2-68 (also known as Flaming Skull Nebula) is a planetary nebula located in the constellation Serpens. It is the remnant of a low to intermediate mass
Sh_2-68
Emission nebula in Cassiopeia constellation
labels it as a G5 star. The nebula contains a total of 71 variable stars. Sh 2-170 has a magnitude of about 6.5. It is best viewed with a hydrogen-alpha
Sh_2-170
Emission nebula
Sh 2-12 is an emission nebula in Scorpius. It was discovered by Stewart Sharpless in 1951 as he began to work on his catalog of nebulae, which would become
Sh_2-12
Planetary nebula in the constellation Cygnus
Sh 2-113 (Sharpless 113) also known as the Flying Dragon Nebula or LBN 333, is a nebula that resembles a supernova remnant (SNR) but with no evidence to
Sh_2-113
Molecular cloud in the constellation Canis Major
Sh 2-310 is a nebula in the slightly southern constellation of Canis Major. It is one of the largest H II regions known in the Milky Way. It is ionized
Sh_2-310
Emission nebula in the constellation Cygnus
listed the two nebulae together in his second list of 313 bright nebulae as Sh 2-117. American astronomer Beverly T. Lynds catalogued the obscuring dust cloud
North_America_Nebula
HII Region in Scorpius
Sh 2-2, also known as Sharpless 2, is an emission nebula in the constellation of Scorpius. It appears as a mid-range brightness making it difficult to
Sh_2-2
Emission nebula in the Cepheus constellation
edu. "Emission Nebula Sh2-140". www.noirlab.edu. Retrieved 2024-09-07. "Sh 2-140". galaxymap.org. Retrieved 2024-09-07. "APOD: 2004 May 20 - Sharpless
Sh_2-140
Interstellar cloud in Orion
Sh 2-1 Sh 2-2 Sh 2-3 Sh 2-4 Sh 2-5 Sh 2-6 Sh 2-7 Sh 2-8 Sh 2-9 Sh 2-10 Sh 2-11 Sh 2-12 Sh 2-13 Sh 2-14 Sh 2-15 Sh 2-16 Sh 2-17 Sh 2-18 Sh 2-19 Sh 2-20
Sh_2-264
H II region
Sh 2-46 (also known as RCW 158), is an H II region, a glowing cloud of ionized hydrogen gas—located in the southern constellation of Serpens. Situated
Sh_2-46
Emission nebula in constellation Ophiuchus
Sh 2-27 (also known as the Cobold Nebula or the Zeta Ophiuchi Nebula), is an emission nebula in the constellation Ophiuchus. It is ionized by the star
Sh_2-27
Molecular cloud
Sh 2-36 is a molecular cloud in Serpens. It is very faint and requires very dark skies to become visible. "Sh 2-36". "Sharpless (Sh2) - Astrobasics".
Sh_2-36
Emission nebula
Sh 2-4 is an emission nebula in the constellation Scorpius. It is part of the Sharpless Catalog assembled by Stewart Sharpless. It was originally misidentified
Sh_2-4
Emission nebula in the constellation Cygnus
Sh 2-106, also known as the Celestial Snow Angel, is an emission nebula and a star formation region in the constellation Cygnus. It is a H II region estimated
Sh_2-106
Emission nebula
Sh 2-14 is an emission nebula in Scorpius. It is ionized by the supergiant HD 158618 and the giant HD 159090. It is possible Stewart Sharpless initially
Sh_2-14
Emission nebula in Lacerta constellation
Sh 2-126 (also known as Great Lacerta Nebula or Star Funnel Nebula) is a large emission nebula and molecular cloud complex located approximately 1200 light-years
Sh_2-126
Nebula in the constellation Serpens
Sh 2-54 is an extended bright nebula in the constellation of Serpens. In its core there are many protostars and many infrared sources; some of these sources
Sh_2-54
Nebula
Sh 2-294, also known as the Octopus Nebula, is a nebula in Monoceros. It was discovered by Wolfgang Strohmeier in 1950, during a photographic survey. It
Sh_2-294
Emission nebula
Stewart Sharpless. It lies next to the Sharpless objects Sh 2-15, Sh 2-16, Sh 2-17, Sh 2-18, and Sh 2-19. It contains the two infrared clusters, [DB2000] 5
Sh_2-20
Molecular cloud
Sh 2-307 is a nebula in Puppis. It contains the potential infrared cluster [DBS2003] 8. It is located in the Perseus Arm. Although appearing small visuallly
Sh_2-307
Emission nebula
Sh 2-44 is a nebula in Sagittarius. It is also known by the designation IC 4701. It is located in the Sagittarius arm of the milky way. NGC 6596 is an
Sh_2-44
Emission nebula
Sh 2-17 is an emission nebula in the constellation Sagittarius. It is part of the Sharpless Catalog assembled by Stewart Sharpless. It contains the infrared
Sh_2-17
Emission nebula
Sh 2-50 is an emission nebula in Scutum. It is located only 2.5° away from the Eagle Nebula. It is in the direction of the open cluster Dolidze 28. It
Sh_2-50
Molecular cloud
Sh 2-34, also known as the Forgotten Nebula is a nebula in Sagittarius. It is a star-forming region and contains multiple filamentary structures. Most
Sh_2-34
Constellation in the northern celestial hemisphere
distance of about 5,650 ly (1,700 pc). Near Eta Cygni, the Tulip nebula (Sh 2-101) and the Cygnus X-1 nebula are located. The latter is formed by jets ejected
Cygnus_(constellation)
HII Region
Sh 2-9, also known as Gum 65, is combination emission and reflection nebula in the Scorpius constellation, surrounding the multiple star system Sigma Scorpii
Sh_2-9
Reflection nebula in the Sagitta constellation
Sh 2-82 (also known as the Little Cocoon Nebula or Little Trifid Nebula) is a small H II region and reflection nebula located in the constellation Sagitta
Sh_2-82
Molecular cloud
Sh 2-23 is a molecular cloud in the constellation Scorpius. It is part of the Sharpless Catalog assembled by Stewart Sharpless. It is located nearby to
Sh_2-23
Planetary nebula
Sh 2-71 is a planetary nebula in the constellation of Aquila. It is notable for its highly irregular and complex morphology, which has been attributed
Sh_2-71
Nebula
Sh 2-10, also called RCW 130, is an emission nebula in the Scorpius constellation. For unknown reasons, it is a significant source of radio emissions.
Sh_2-10
Nebula
Sh 2-1, also known as Sharpless 1, is the combination of a diffuse HII emission nebula and reflection nebula in the constellation of Scorpius with Pi Scorpii
Sh_2-1
Molecular cloud
Sh 2-41 is a large nebula in Sagittarius and a component of the Small Sagittarius Star Cloud Sh 2-41 appears near the northern edge of the star cloud
Sh_2-41
Open cluster in the constellation Serpens
million times that of the Sun. The cluster's age has been estimated to be 1–2 million years. The descriptive names reflect impressions of the shape of the
Eagle_Nebula
Emission nebula
star's corresponding ring nebula around it are unrelated to Sh 2-22. "Sh 2-22". "Sharpless (Sh2) - Astrobasics". 13 September 2022. "Sh 2-22". v t e
Sh_2-22
Emission nebula
Sh 2-16 is an emission nebula in the constellation Sagittarius. It is ionized by the star LSS 4381. The nebula also contains an infrared cluster, [DB2000]
Sh_2-16
Emission nebula in the constellation Cygnus
temperatures. The Crescent Nebula is a rather small object located about 2 degrees Southwest of Sadr. While considered bright by astronomical imaging
Crescent_Nebula
Molecular cloud
Sh 2-306 (also designated RCW 10), is an emission nebula and H II region located in the southern constellation Puppis. It is catalogued in the Sharpless
Sh_2-306
Emission nebula and H II region
stars [VM75] Sh 2-305 4 (O8.5V) and [VM75] Sh 2-305 2 (O9.5V) accompanied by a pair of B-type stars [VM75] Sh 2-305 7 (B0V) and [VM75] Sh 2-305 8 (B0V)
Sh_2-305
Emission nebula
Sh 2-38 is a nebula in the constellation Sagittarius. It appears in the shape of a bubble. "SIMBAD query result". Blitz, L.; Fich, M.; Stark, A. A. (1982)
Sh_2-38
Molecular cloud
Sh 2-40 is a large nebula in Sagittarius. It is just north of Sh 2-41. Sh 2-40 is in the same direction as powerful radio source W 33. W 33 is, however
Sh_2-40
Emission nebula
Sh 2-15 is an emission nebula in the constellation of Scorpius. It is ionized by the star HD 161853. It is most visible using a Hydrogen-alpha filter.
Sh_2-15
Emission nebula
Nebula, listed in the Sharpless catalog as Sh 2-11, and Sh 2-5 itself contains NGC 6337. Like the nearby Sh 2-4, Sh 2-5 is probably ionized by the nearby star
Sh_2-5
Emission nebula
Sh 2-32, also known by the designation IC 1274, is an emission nebula in the constellation Sagittarius. It is a major source of gamma rays. Sh 2-32 was
Sh_2-32
Emission nebula
Sh 2-13 is an emission nebula in Scorpius. It is ionized by nearby star HD 158186. Sh 2-13 also contains a star cluster it has formed, Antalova 1. It
Sh_2-13
Nebula in the constellation Vulpecula
Sharpless 2-88 or Sh 2-88 is a region including the diffuse nebula Sh 2-88A and the two compact knots Sh 2-88B1 and Sh 2-88B2, all of which are associated
Sh_2-88
Emission nebula
Sh 2-19 is an emission nebula in the constellation Sagittarius. It is part of the Sharpless Catalog assembled by Stewart Sharpless. It lies next to Sh
Sh_2-19
Emission nebula in the constellation of Orion
Barnard's Loop (catalogue designation Sh 2-276) is an emission nebula in the constellation of Orion. It is part of the Orion–Eridanus Superbubble, which
Barnard's_Loop
Emission nebula in Sagittarius
Vicinity". In Bo Reipurth (ed.). Handbook of Star-Forming Regions: Volume 2 The Southern Sky. Astronomical Society of the Pacific. p. 53. ISBN 978-1-58381-671-4
Lagoon_Nebula
Cloud of heated and ionized gas and dust in the constellation Cygnus
the western end of the nebula as "Extended; passes thro' 52 Cygni... near 2 degree in length", and described the eastern end as "Branching nebulosity
Veil_Nebula
Emission nebula
HD 165921 and HD 166107. Sh 2-31 is located very close to the Lagoon Nebula. Sh 2-31 was discovered, along with nearby Sh 2-29, by John Herschel on 1st
Sh_2-31
Emission nebula in Scorpius
Sh 2-7 is an emission nebula in the Scorpius constellation. The nebula is around the star Delta Scorpii. It lies next to a large reflection nebula, Sh
Sh_2-7
Diffuse nebula
Sh 2-48 is a diffuse nebula in Scutum. It is often overlooked due to proximity to the much more famous Eagle Nebula. The open cluster Kronberger 25 is
Sh_2-48
Reflection nebula in the constellation Cygnus
IC 5146 (also Caldwell 19, Sh 2-125, Barnard 168, and the Cocoon Nebula) is a reflection/emission nebula and Caldwell object in the constellation Cygnus
IC_5146
X-ray binary in Cygnus containing a stellar black hole
sources detectable from Earth, producing a peak X-ray flux density of 2.3×10−23 W/(m2⋅Hz) (2.3×103 jansky). It remains among the most studied astronomical objects
Cygnus_X-1
Molecular cloud
Sh 2-24 is a molecular cloud in the constellation Ophiuchus, near the border with Scorpius. It is part of the Sharpless catalog assembled by Stewart Sharpless
Sh_2-24
Supernova remnant
remnant in Cygnus. It is made up of multiple Sharpless Objects. Sh 2-92, Sh 2-94, and Sh 2-96. The nebula was discovered in 1977 during an optical study
SNR_G65.3+5.7
Molecular cloud
Sh 2-35 is a nebula in Sagittarius. It is best viewed with a Hydrogen-alpha filter. It is located near to Sh 2-37. combined with Sh 2-37, it has a mass
Sh_2-35
Blue supergiant star in the constellation Cygnus
highest value, it is the farthest star with an apparent magnitude brighter than 2.50. α Cygni (Greco-Latinised to Alpha Cygni) is the star's designation given
Deneb
Emission nebula
Sh 2-43 also known as RCW 156, is an emission nebula located in the constellation of Sagittarius. It is a faint, diffuse region of ionized hydrogen gas
Sh_2-43
Molecular cloud
Sh 2-47 is a nebula in Serpens. It is probably ionized by the star [L85] S47 3. It is located between Messier 17 and Sh 2-44. "Sh 2-47". "CCD Images of
Sh_2-47
Nebula
Sh 2-87 is a star-forming nebula with a mass of about 7000 suns. It is close to Sh 2-88, and is located in the central part of the constellation Vulpecula
Sh_2-87
Planetary nebula
Sh 2-42 is a planetary nebula in Sagittarius. It is included in the Sharpless catalogue, however the position indicated by the original catalogue was one
Sh_2-42
Star noted for unusual dimming events
had a pattern similar to the one at 759.75 days from the Kepler event 2, epoch 2 data. Observations were taken across the electromagnetic spectrum. Evidence
Tabby's_Star
Planetary nebula
Sh 2-78 is a planetary nebula in Aquila. It was discovered by Stewart Sharpless while assembling his catalogue, and identified as a planetary nebula in
Sh_2-78
Emission nebula
Sh 2-21 is an emission nebula in the constellation Sagittarius. It is part of the Sharpless Catalog assembled by Stewart Sharpless. It is associated with
Sh_2-21
Emission nebula
Sh 2-18 is an emission nebula in the constellation Sagittarius. It is part of the Sharpless Catalog assembled by Stewart Sharpless. It lies next to Sh
Sh_2-18
Emission nebula
Sh 2-297 (also known as Sharpless 297) is an emission nebula in the constellation Canis Major. The region was catalogued in 1959 in the extended seconded
Sh_2-297
Made of a list
Sh 2-1 Sh 2-2 Sh 2-3 Sh 2-4 Sh 2-5 Sh 2-6 Sh 2-7 Sh 2-8 Sh 2-9 Sh 2-10 Sh 2-11 Sh 2-12 Sh 2-13 Sh 2-14 Sh 2-15 Sh 2-16 Sh 2-17 Sh 2-18 Sh 2-19 Sh 2-20
Sharpless_catalog
Emission nebula
The Clamshell Nebula (also known as Sh 2-119) is an emission nebula and star-forming region located in the constellation Cygnus. The Clamshell Nebula was
Clamshell_Nebula
Molecular Cloud
Sh 2-33 is a molecular cloud in Serpens. It has also been described as a dark globule. It is very faint and has very little color, and must be observed
Sh_2-33
Planetary nebula in the constellation Cygnus
planetary nebula by Heber Doust Curtis in 1919. The central star is magnitude 16.2 Curtis, H.D. "Three New Planetary Nebulae". Steinecke, Wolfgang. "Revised
NGC_6842
Emission nebula in the constellation Sagittarius
Islands (King Crimson album), which uses an image of the nebula as its cover Sh 2-82, also known as the 'Little Trifid Nebula' NGC 1579, also known as the
Trifid_Nebula
Star in the constellation Cygnus
(February 2012). "Kepler-22b: A 2.4 Earth-radius Planet in the Habitable Zone of a Sun-like Star". The Astrophysical Journal. 745 (2): 120. arXiv:1112.1640. Bibcode:2012ApJ
Kepler-22
Molecular cloud
Sh 2-309 is a nebula in Puppis. The nebula contains the infrared cluster [DBS2003] 9. It is located beyond the Carina Arm. Sh 2-308 is ionized by the
Sh_2-309
Disappearing red supergiant star in the galaxy NGC 6946
of the star, given by its apparent magnitude in different colour bands on 2 July 2005 is given by R = 21, V = 22, B = 23, U = 24. Prior to the optical
N6946-BH1
Supernova remnant in the constellation of Cygnus
loop at 34.5 MHz". Journal of Astrophysics and Astronomy. 2 (3): 339–347. Bibcode:1981JApA....2..339S. doi:10.1007/BF02714557. ISSN 0250-6335. S2CID 55053690
Cygnus_Loop
Molecular cloud
Sh 2-312 is a nebula in the southern constellation of Pyxis. It is very large and diffuse, making it largely ignored and unstudied outside of its relation
Sh_2-312
Hot Jovian exoplanet orbiting KELT-9
exoplanet. The host star, KELT-9, also designated HD 195689, is 2.3 times larger and 2.4 times more massive than the sun. The surface temperature is 10
KELT-9b
Double star system in the constellation Cygnus
In 1976 speckle interferometry was used to resolve a companion using the 2.1-meter telescope at the Kitt Peak National Observatory. It was measured at
Albireo
Gas giant orbiting Kepler-1625
result of the star's slightly greater mass than the Sun. Kepler-1625b receives 2.6 times more insolation than the Earth, meaning it lies at the inner edge
Kepler-1625b
Star in the constellation of Cygnus
causing WR 142 to lose roughly 1.6×10−5 M☉/year. For comparison, the Sun loses (2–3)×10−14 M☉/year due to its solar wind, several hundred million times less
WR_142
G-type main-sequence star in the constellation Cygnus
Astronomical Journal. 105 (2). Institute of Physics: 56. arXiv:1507.06723. Bibcode:2015AJ....150...56J. doi:10.1088/0004-6256/150/2/56. S2CID 26447864. "Kepler-452"
Kepler-452
Emission nebula in the constellation Perseus
as the latitude matches the declination of the object. NGC 1499 is almost 2.5° long on the sky and, because of its very low surface brightness, it is
California_Nebula
Star in the constellation Cygnus
The Astrophysical Journal. 835 (2): 239. arXiv:1612.01598. Bibcode:2017ApJ...835..239S. doi:10.3847/1538-4357/835/2/239. S2CID 73634716. "Kepler-186
Kepler-186
Molecular cloud
"NGC 6857 - HII Ionized region in Cygnus". "Sh 2-99". "Sh 2-100". "Galactic Nebulae NGC 6857 (Sh 2-100) + Sh 2-99". "NOTES FROM OBSERVATION II. NGC 6857"
NGC_6857
Star formation region in the constellation of Cygnus
spectral type OB and a mass of up to 105 solar masses) within a radius of 2 kiloparsecs of the Sun. It is also associated with one of the largest molecular
Cygnus_X_(star_complex)
Diffuse nebula in the constellation Orion
232L. Schreiber, John (1904). "Jesuit Astronomy". Popular Astronomy. 12: 101. Harrison, Thomas G. (1984). "The Orion Nebula: Where in History is it?"
Orion_Nebula
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