AI & ChatGPT searches , social queries for BOLOMETRIC CORRECTION
Search references for BOLOMETRIC CORRECTION. Phrases containing BOLOMETRIC CORRECTION
See searches and references containing BOLOMETRIC CORRECTION!
Search references for BOLOMETRIC CORRECTION. Phrases containing BOLOMETRIC CORRECTION
See searches and references containing BOLOMETRIC CORRECTION!BOLOMETRIC CORRECTION
Calculation in astronomy
the bolometric correction is the correction made to the absolute visual magnitude of an object in order to convert it to an absolute bolometric magnitude
Bolometric_correction
Measurement of radiant electromagnetic power emitted by an object
star observed only in the infrared. Bolometric luminosities can also be calculated using a bolometric correction to a luminosity in a particular passband
Luminosity
Calibration factor in a photometric system
and apparent bolometric magnitude zero points to be 3.0128×1028 W and 2.51802×10−8 W/m2, respectively. Luminosity Bolometric correction Absolute magnitude
Zero_point_(photometry)
Measure of the luminosity of celestial objects
absolute magnitude in a specific filter band to absolute bolometric magnitude, a bolometric correction (BC) is applied. In stellar and galactic astronomy,
Absolute_magnitude
the bolometric magnitude 4.54 ± 0.06 and the bolometric correction −0.12 ± 0.05 using the formula: BC = Mbol − MV Calculated from the bolometric magnitude
List of nearest stars by spectral type
List_of_nearest_stars_by_spectral_type
Star system in the constellation Ursa Major
the bolometric magnitude 4.54 ± 0.06 and the bolometric correction −0.12 ± 0.05 using the formula: BC = Mbol − MV Calculated from the bolometric magnitude
Xi_Ursae_Majoris
Type of star that is massive and luminous
bolometric luminosity is much higher than the visual luminosity, sometimes several magnitudes or a factor of five or more. This bolometric correction
Supergiant
Stars sorted by absolute magnitude
each star, and a correction for interstellar extinction. The entries in the list below are further corrected to provide the bolometric magnitude, i.e.
List_of_most_luminous_stars
Scatter plot of stars showing the relationship of luminosity to stellar classification
converting luminosity or absolute bolometric magnitude to apparent or absolute visual magnitude, one requires a bolometric correction, which may or may not come
Hertzsprung–Russell_diagram
Wolf–Rayet star in the constellation Dorado
99% of the radiation to be emitted outside the visual range (a bolometric correction around −5). R136a1 is over forty times the radius of the Sun (42
R136a1
Dim, low mass stars on the main sequence
Eric E. (1 September 2013). "Intrinsic Colors, Temperatures, and Bolometric Corrections of Pre-main-sequence Stars". The Astrophysical Journal Supplement
Red_dwarf
Stellar classification
; Mamajek, Eric E. (2013). "Intrinsic Colors, Temperatures, and Bolometric Corrections of Pre-main-sequence Stars". The Astrophysical Journal Supplement
K-type_main-sequence_star
Stellar classification
Eric E. (1 September 2013). "Intrinsic Colors, Temperatures, and Bolometric Corrections of Pre-main-sequence Stars". The Astrophysical Journal Supplement
G-type_main-sequence_star
Red giant in the constellation Volans
995, distance modulus 16.9, G-band extinction 0.397, and G-band bolometric correction −0.568 Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia
SDSS_J0715-7334
Stellar classification
Eric E. (1 September 2013). "Intrinsic Colors, Temperatures, and Bolometric Corrections of Pre-main-sequence Stars". The Astrophysical Journal Supplement
F-type_main-sequence_star
Brightest star in the constellation of Carina
but white to him. The bolometric correction for Canopus is 0.00, indicating that the visual absolute magnitude and bolometric absolute magnitude are
Canopus
Formula for measuring astronomical objects
estimate K corrections to these measurements in order to make comparisons. If one could measure all wavelengths of light from an object (a bolometric flux)
K_correction
Lightest color
by B.W Caroll and D.A Ostlie 1996 edition, chapter 8 Empirical bolometric corrections for the main-sequence Archived 9 November 2017 at the Wayback Machine
White
Star in the constellation Libra
that humans are able to see), something known as the bolometric correction, this star has a bolometric luminosity 1.2% of the Sun's total luminosity. A planet
Gliese_581
Stellar classification
Eric E. (1 September 2013). "Intrinsic Colors, Temperatures, and Bolometric Corrections of Pre-main-sequence Stars". The Astrophysical Journal Supplement
A-type_main-sequence_star
Binary star located in the Small Magellanic Cloud in the constellation Hydrus
luminosity and apply a bolometric correction to give the total luminosity at all wavelengths, although the size of the bolometric correction is extremely sensitive
AB8_(star)
Stellar classification distinguished by bright blue luminosity
Eric E. (1 September 2013). "Intrinsic Colors, Temperatures, and Bolometric Corrections of Pre-main-sequence Stars". The Astrophysical Journal Supplement
B-type_main-sequence_star
ISSN 0004-637X. Nieva, M.-F. (2013). "Temperature, gravity, and bolometric correction scales for non-supergiant OB stars". Astronomy & Astrophysics. 550:
List_of_most_massive_stars
Star at the centre of the Solar System
Castelli, F.; Plez, B. (1998). "Model atmospheres broad-band colors, bolometric corrections and temperature calibrations for O–M stars". Astronomy and Astrophysics
Sun
Main-sequence star of spectral type O
Eric E. (1 September 2013). "Intrinsic colors, temperatures, and bolometric corrections of pre-main-sequence stars". The Astrophysical Journal Supplement
O-type_main-sequence_star
Star noted for unusual dimming events
Eric E. (September 2013). "Intrinsic Colors, Temperatures, and Bolometric Corrections of Pre-main-sequence Stars". The Astrophysical Journal Supplement
Tabby's_Star
Binary star in the Small Magellanic Cloud in the constellation Tucana
luminosity and apply a bolometric correction to give the total luminosity at all wavelengths, although the size of the bolometric correction is extremely sensitive
AB7
1987 supernova event in the constellation Dorado
supernova remnants Lyman, J. D.; Bersier, D.; James, P. A. (2013). "Bolometric corrections for optical light curves of core-collapse supernovae". Monthly Notices
SN_1987A
Binary star in the constellation Cepheus
175B. Habets, G. M. H. J.; Heintz, J. R. W. (1981). "Empirical bolometric corrections for the main-sequence". Astronomy and Astrophysics Supplement Series
VV_Cephei
Classification of stars based on spectral properties
Habets, G. M. H. J.; Heinze, J. R. W. (November 1981). "Empirical bolometric corrections for the main-sequence". Astronomy and Astrophysics Supplement Series
Stellar_classification
{\displaystyle B-V=M_{B}-M_{V}\!\,} dimensionless dimensionless Bolometric correction Cbol (No standard symbol) C b o l = m b o l − V = M b o l − M V
List_of_optics_equations
Star in the constellation Lepus
S2CID 18759600. Nieva, M.-F. (February 2013), "Temperature, gravity, and bolometric correction scales for non-supergiant OB stars", Astronomy & Astrophysics, 550:
Lambda_Leporis
Star in the constellation Orion
VizieR. Nieva, M.-F. (February 2013). "Temperature, gravity, and bolometric correction scales for non-supergiant OB stars". Astronomy & Astrophysics. 550:
Upsilon_Orionis
Brightest star in the constellation Auriga
730±60 K for Ab. Their bolometric luminosities are most accurately derived from their apparent magnitudes and bolometric corrections, but are confirmed by
Capella
Star in the constellation Camelopardalis
; Jordi, C.; Ribas, I. (2006). "Effective temperature scale and bolometric corrections from 2MASS photometry". Astronomy and Astrophysics. 450 (2): 735
21_Camelopardalis
Star in the constellation Sagittarius
K-band magnitude of 7.89, a K-band extinction of 1.7, and a K-band bolometric correction of -2.9, the luminosity turns out to be 2.4 million times that of
WR_101-2
Leeuwen theorem Bohumil Kučera Boiling point Boilover Bolometer Bolometric correction Boltzmann's entropy formula Boltzmann-Matano analysis Boltzmann
Index_of_physics_articles_(B)
F-type main sequence star in the constellation Eridanus
; Mamajek, Eric E. (2013). "Intrinsic Colors, Temperatures, and Bolometric Corrections of Pre-main-sequence Stars". The Astrophysical Journal Supplement
51_Eridani
K-type star in the constellation Pictor
database J/A+A/450/735; described in Effective temperature scale and bolometric corrections from 2MASS photometry, E. Masana, C. Jordi, and I. Ribas, Astronomy
HD_40307
Brightness of a celestial object observed from the Earth
apparent bolometric magnitude scale is based on the International Astronomical Union 2015 Resolution B2, which defines an apparent bolometric magnitude
Apparent_magnitude
Star in the constellation Centaurus
beginning of the 20th century to 13.2 in 2010 (due to changes in the bolometric correction), while its radius is calculated to have decreased from 100 R☉ to
DY_Centauri
American astrophysicist
; Mamajek, Eric E. (2013). "Intrinsic Colors, Temperatures, And Bolometric Corrections of Pre-Main-Sequence Stars". The Astrophysical Journal Supplement
Eric_Mamajek
K-type subgiant star in the constellation Pisces
Eric E. (1 September 2013). "Intrinsic Colors, Temperatures, and Bolometric Corrections of Pre-main-sequence Stars". The Astrophysical Journal Supplement
HD_30856
Variable star in the constellation Eridanus
S2CID 18759600. Nieva, M.-F. (February 2013), "Temperature, gravity, and bolometric correction scales for non-supergiant OB stars", Astronomy & Astrophysics, 550:
Nu_Eridani
Star in the constellation Centaurus
VizieR. Nieva, M.-F. (February 2013). "Temperature, gravity, and bolometric correction scales for non-supergiant OB stars". Astronomy & Astrophysics. 550:
Chi_Centauri
G-dwarf star w. a planet; Corona Australis
C.; Ribas, I. (10 April 2006). "Effective temperature scale and bolometric corrections from 2MASS photometry". Astronomy & Astrophysics. 450 (2): 735–746
HD_177565
F-type star with a circumstellar disk
C.; Ribas, I. (10 April 2006). "Effective temperature scale and bolometric corrections from 2MASS photometry". Astronomy & Astrophysics. 450 (2): 735–746
HD_180134
Star system in the constellation Draco
E; Jordi, C; Ribas, I (2006). "Effective temperature scale and bolometric corrections from 2MASS photometry". Astronomy & Astrophysics. 450 (2): 735.
Nu_Draconis
F-type main-sequence star in Triangulum
C.; Ribas, I. (10 April 2006). "Effective temperature scale and bolometric corrections from 2MASS photometry". Astronomy & Astrophysics. 450 (2): 735–746
HD_11007
List of largest planets by size
Castelli, F.; Plez, B. (1998). "Model atmospheres broad-band colors, bolometric corrections and temperature calibrations for O–M stars". Astronomy and Astrophysics
List_of_largest_exoplanets
High proper motion star; F-type dwarf
C.; Ribas, I. (10 April 2006). "Effective temperature scale and bolometric corrections from 2MASS photometry". Astronomy & Astrophysics. 450 (2): 735–746
HD_192886
G-type main sequence star; Telescopium
C.; Ribas, I. (10 April 2006). "Effective temperature scale and bolometric corrections from 2MASS photometry". Astronomy & Astrophysics. 450 (2): 735–746
HD_168871
Star in the constellation Canis Minor
E; Jordi, C; Ribas, I (2006). "Effective temperature scale and bolometric corrections from 2MASS photometry". Astronomy & Astrophysics. 450 (2): 735.
Delta2_Canis_Minoris
Star in the constellation Microscopium
C.; Ribas, I. (10 April 2006). "Effective temperature scale and bolometric corrections from 2MASS photometry". Astronomy & Astrophysics. 450 (2): 735–746
HD_201772
Star in the constellation Taurus
S2CID 119257644. Masana, E.; et al. (2006), "Effective temperature scale and bolometric corrections from 2MASS photometry", Astronomy and Astrophysics, 450 (2): 735
Omega2_Tauri
Star in the constellation Leo Minor
S2CID 119231169. Masana, E.; et al. (2006). "Effective temperature scale and bolometric corrections from 2MASS photometry". Astronomy and Astrophysics. 450 (2): 735
30_Leonis_Minoris
Star in the constellation of Caelum
C.; Ribas, I. (10 April 2006). "Effective temperature scale and bolometric corrections from 2MASS photometry". Astronomy & Astrophysics. 450 (2): 735–746
HD_32820
Astrometric binary in the constellation Telescopium
C.; Ribas, I. (10 April 2006). "Effective temperature scale and bolometric corrections from 2MASS photometry". Astronomy & Astrophysics. 450 (2): 735–746
HD_181295
Anti-tank guided missile
The new system features a new, non-cooled thermal sight which uses a bolometric sensor. MBDA asserts that the new sight is quieter, reduces weight, increases
Eryx_(missile)
Northern pole-star; brightest star in Ursa Minor
is 136.9±0.3 pc (446.5±1.1 ly) using the baseline parallax zeropoint correction. Gaia DR4 (expected December 2026) will further improve the statistical
Polaris
Red supergiant star in the constellation Orion
effective temperature and bolometric luminosity. The Rosseland radius differs from directly measured radii, with corrections for limb darkening and the
Betelgeuse
NASA spacecraft (2006–present)
nitriles in the atmosphere Search for any Charon atmosphere Determine bolometric Bond albedos for Pluto and Charon Map surface temperatures of Pluto and
New_Horizons
in the sky as seen at frequencies above 1 GHz Sombrero Galaxy 1×109 Bolometrically most luminous galaxy in the local universe and also the nearest billion-solar-mass
List of most massive black holes
List_of_most_massive_black_holes
star's singly ionized calcium H and K lines, after correction for photospheric light, to the bolometric flux. Schröder et al. (2009) divide solar-type stars
Glossary_of_astronomy
Trace radiation from the early universe
"Optical design of the Atacama Cosmology Telescope and the Millimeter Bolometric Array Camera". Applied Optics. 46 (17): 3444–3454. arXiv:astro-ph/0701020
Cosmic_microwave_background
Red dwarf star in the constellation Aquarius
Kitzmann, Daniel; Heng, Kevin (20 January 2025). "Stellar Contamination Correction Using Back-to-back Transits of TRAPPIST-1 b and c". The Astrophysical
TRAPPIST-1
Stellar system in the constellation Carina
normal outburst are visually brighter than when quiescent although the bolometric luminosity is unchanged. An event similar to η Carinae A's Great Eruption
Eta_Carinae
Binary star system in the constellation Draco
white dwarf star. The measured angular diameter of the primary, after correction for limb darkening, is 1.69±0.02 mas. At the estimated distance of Upsilon
Upsilon_Draconis
Star in the constellation Virgo
Hevelius, Deduced from the Best Authorities. With Various Notes and Corrections, and a Preface to Each Catalogue. To Which is Added the Synonym of each
59_Virginis
BOLOMETRIC CORRECTION
BOLOMETRIC CORRECTION
BOLOMETRIC CORRECTION
BOLOMETRIC CORRECTION
BOLOMETRIC CORRECTION
BOLOMETRIC CORRECTION
BOLOMETRIC CORRECTION
BOLOMETRIC CORRECTION
BOLOMETRIC CORRECTION