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From Wikipedia, the free encyclopedia

Trumpler 27-1

The Trumpler 27 open cluster. Trumpler 27-1 is the brightest and reddest star in the image.
Observation data
Epoch J2000      Equinox J2000
Constellation Scorpius
Right ascension 17h 36m 10.1193s[1]
Declination −33° 29′ 40.617″[1]
Apparent magnitude (V) 8.79[2]
Characteristics
Evolutionary stage Red supergiant
Spectral type M0Ia[2]
Astrometry
Radial velocity (Rv)−18.71±0.9[1] km/s
Proper motion (μ) RA: −0.057±0.049 mas/yr[1]
Dec.: −1.386±0.037 mas/yr[1]
Parallax (π)0.3169 ± 0.0361 mas[1]
Distanceapprox. 10,000 ly
(approx. 3,200 pc)
Details[3]
Radius1,359 R
Luminosity361,000 L
Surface gravity (log g)-0.24[4] cgs
Temperature3,790 K
Metallicity [Fe/H]+0.15[4] dex
Other designations
CD−33 12241, CPD−33 4468, TYC 7380-627-1[2]
Database references
SIMBADdata

Trumpler 27-1 is a red supergiant star that is a member of the massive, possible open cluster Trumpler-27, where a blue giant star, a yellow supergiant star, and two Wolf–Rayet stars are also located.

Observation history

Trumpler 27-1 was discovered and catalogued when the open cluster (not confirmed then) was first identified in the late 20th century.[citation needed] It has since remained largely unobserved, being featured in the Gaia Catalogue and other pieces of literature.[5]

Physical properties

Trumpler 27-1 is among the largest stars known, with a radius of over 1,360 solar radii. It is also 360,000 times more luminous than the Sun.[3] This star's spectral type is M0Ia,[6] meaning it possesses a cool temperature of below 3,800 K. So far, Trumpler 27-1 is the only identified red supergiant in the open cluster Trumpler 27.[citation needed]

Location

Trumpler 27–1, and the open cluster in which it is located, is in the constellation of Scorpius.

See also

References

  1. ^ a b c d e Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
  2. ^ a b c "CD-33 12241". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 17 July 2020.
  3. ^ a b Healy, Sarah; Horiuchi, Shunsaku; Molla, Marta Colomer; Milisavljevic, Dan; Tseng, Jeff; Bergin, Faith; Weil, Kathryn; Tanaka, Masaomi (23 March 2024). "Red Supergiant Candidates for Multimessenger Monitoring of the Next Galactic Supernova". Monthly Notices of the Royal Astronomical Society. 529 (4): 3630–3650. arXiv:2307.08785. Bibcode:2024MNRAS.529.3630H. doi:10.1093/mnras/stae738. ISSN 0035-8711.
  4. ^ a b Anders, F.; Khalatyan, A.; Chiappini, C.; Queiroz, A. B.; Santiago, B. X.; Jordi, C.; Girardi, L.; Brown, A. G. A.; Matijevič, G.; Monari, G.; Cantat-Gaudin, T.; Weiler, M.; Khan, S.; Miglio, A.; Carrillo, I.; Romero-Gómez, M.; Minchev, I.; De Jong, R. S.; Antoja, T.; Ramos, P.; Steinmetz, M.; Enke, H. (2019). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18". Astronomy and Astrophysics. 628: A94. arXiv:1904.11302. Bibcode:2019A&A...628A..94A. doi:10.1051/0004-6361/201935765. S2CID 131780028.
  5. ^ Stassun, Keivan G.; et al. (1 October 2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138. arXiv:1905.10694. Bibcode:2019AJ....158..138S. doi:10.3847/1538-3881/ab3467. hdl:1721.1/124721. ISSN 0004-6256. S2CID 166227927.
  6. ^ Messineo, M.; Brown, A. G. A. (2019). "A Catalog of Known Galactic K-M Stars of Class I Candidate Red Supergiants in Gaia DR2". The Astronomical Journal. 158 (1): 20. arXiv:1905.03744. Bibcode:2019AJ....158...20M. doi:10.3847/1538-3881/ab1cbd. S2CID 148571616.
This page was last edited on 13 June 2024, at 15:20
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