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Hypergiant star in the constellation Aquila
IRC +10420, also known as V1302 Aquilae, is a yellow hypergiant star located in the constellation of Aquila at a distance of 4-6 kiloparsecs of the Sun
IRC_+10420
Topics referred to by the same term
which have the form IRC followed by a five-digit number, standing for infrared catalogue IRC -10414, a red supergiant star IRC +10420, a yellow hypergiant
IRC_(disambiguation)
Rare star with tremendous luminosity and high rates of mass loss by stellar winds
LMC) HD 74180 HD 268757 (R59 in LMC) IRAS 17163-3907 IRAS 18357-0604 IRC+10420 (V1302 Aql) Omicron1 Centauri Phi Cassiopeiae R Puppis Rho Cassiopeiae
Hypergiant
Star in the constellation Canis Major
that around the post-red supergiant yellow hypergiant (Post-RSG YHG) IRC +10420. The similarity has led studies proposing that VY CMa might evolve blueward
VY_Canis_Majoris
Class of massive star with a spectral type of A to K
pseudo-photospheres. Rho Cassiopeiae V509 Cassiopeiae Omicron1 Centauri R Puppis IRC+10420 (V1302 Aql) IRAS 18357-0604 V766 Centauri (= HR 5171A) HD 179821 IRAS
Yellow_hypergiant
Binary star in the constellation Dorado
stars, such as VY Canis Majoris, Mu Cephei, and the post-red supergiant IRC +10420. A much lower luminosity of 280,000 L☉ was derived based on radiative
WOH_G64
Star within the open cluster Stephenson 2
Diagram indicate that it is similar to the extreme yellow hypergiant star IRC+10420 and Variable A in the Triangulum Galaxy (M33). Stephenson 2 DFK 49 is
Stephenson_2_DFK_49
Star in the constellation Scutum
to be considered a true OH/IR supergiant, unlike VY Canis Majoris and IRC +10420. It has some emission-lines and is classified as a semiregular variable
UY_Scuti
doi:10.1086/382218. S2CID 7851916. Jones, Terry Jay; et al. (July 1993). "IRC +10420 - A cool hypergiant near the top of the H-R diagram". The Astrophysical
List_of_supernova_candidates
American stellar astrophyscist
in eta Carinae, and the warm and cool hypergiants such as VY CMa and IRC +10420. She also led the Automated Plate Scanner research group for over twenty
Roberta_M._Humphreys
Classification of stars based on spectral properties
evolutionary void. Three evolutionary critical Hypergiants: HD 33579, HR 8752 & IRC +10420". Astronomy and Astrophysics. 353: 163. Bibcode:2000A&A...353..163N. "On
Stellar_classification
Red supergiant star in the constellation Cepheus
Mid-to-Far Infrared: The Mass Loss Histories of the Hypergiants μ Cep, VY CMa, IRC+10420, and ρ Cas". The Astronomical Journal. 151 (3): 51. arXiv:1512.01529.
Mu_Cephei
; Mackey, J.; Kraus, A.; Meyer, D. M. -A.; Kamiński, T. (January 2014). "IRC −10414: a bow-shock-producing red supergiant star". Monthly Notices of the
List_of_largest_stars
Star in the Triangulum Galaxy
it is present in some other stars with high mass-loss rates, such as IRC +10420. Notably its luminosity is similar to that of LBVs like S Doradus during
B324
Star in the constellation Scutum
years, or 6,000 parsecs, away. IRAS 18357−0604 is remarkably similar to IRC +10420, another yellow hypergiant in the constellation of Aquila. A distance
IRAS_18357−0604
Comparing widely separated telescope wavefronts
Image of the source IRC +10420. The lower resolution image on the left was taken with the UK's MERLIN array and shows the shell of maser emission produced
Very-long-baseline interferometry
Very-long-baseline_interferometry
Hypergiant star in the constellation Cepheus
to be extended, having an azimuthally symmetric structure similar to IRC +10420. The radius of this emission has been estimated to be ~0.3–0.4 arcseconds
RW_Cephei
Mid-to-Far Infrared: The Mass-Loss Histories of the Hypergiants μ Cep, VY CMa, IRC+10420, AND ρ Cas*". The Astronomical Journal. 151 (3): 51. arXiv:1512.01529
List_of_star_extremes
Type of star
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 various
OH/IR_star
Star in the constellation Dorado
evolutionary void. Three evolutionary critical Hypergiants: HD 33579, HR 8752 & IRC +10420". Astronomy and Astrophysics. 353: 163–176 (2000). Bibcode:2000A&A...353
HD_33579
Star in the constellation Aquila
Canis Majoris. Like its constellation neighbor and also hypergiant star IRC +10420, it is surrounded by an extended reflection nebula. Discovered at near-IR
HD_179821
Star in the constellation Cassiopeia
(2013). "Long-term Spectroscopic Monitoring of Cool Hypergiants HR 8752, IRC+10420, and 6 Cas near the Yellow Evolutionary Void". 370 Years of Astronomy
V509_Cassiopeiae
Yellow hypergiant in the constellation Scorpius
properties of these shells are considered similar to those surrounding IRC+10420 (also an evolved massive star suffering heavy mass loss) as well as, for
IRAS_17163−3907
Star in the constellation Aquila
S. (1999). "Spectral atlas of two peculiar supergiants: MWC 314 and IRC +10420". Bulletin of the Special Astrophysical Observatory. 48: 25. arXiv:1602
V1429_Aquilae
Comparison of a wide range of lengths
MID-TO-FAR INFRARED: THE MASS-LOSS HISTORIES OF THE HYPERGIANTS μ Cep, VY CMa, IRC+10420, AND ρ Cas". The Astronomical Journal. 151 (3): 51. arXiv:1512.01529.
Orders_of_magnitude_(length)
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