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HD 300933

From Wikipedia, the free encyclopedia

M-type supergiant in the constellation Vela
HD 300933
Location of HD 300933 (circled)
Observation data
EpochJ2000[1]      EquinoxJ2000[1]
ConstellationVela
Right ascension10h 38m 02.98879s
Declination−56° 49′ 01.9334″
Apparent magnitude (V)8.29[2]
Characteristics
Evolutionary stageRed supergiant
Spectral typeM2 Iab/Ib[3] + B2V[4]
B−Vcolor index+1.70[2]
J−Hcolor index+1.097[5]
J−Kcolor index+1.500[5]
Astrometry
Radial velocity (Rv)−11.05±0.42[6] km/s
Proper motion (μ)RA: −7.461[1]mas/yr
Dec.: 3.539[1]mas/yr
Parallax (π)0.3216±0.0315 mas[1]
Distance3100[7] pc
Details
HD 300933
Radius806[8] R
Temperature3660±170[9] K
Other designations
CD−56°3464,CPD−56°3586,Gaia DR3 5352006438862476288,HD 300933/4,WDS J10380-5649AB,TIC 458199516,TYC 8609-2644-1,GSC 08609-02644,IRAS 10360-5633,2MASS J10380298-5649019,WISE J103803.02-564901.9[10]
Database references
SIMBADdata

HD 300933 (CPD-56°3586) is ared supergiant ofspectral type M2 Iab/Ib[3] in the southernconstellation ofVela, close to the border withCarina. With anapparent magnitude of 8.29, it is too faint to be observed by thenaked eye, but can be seen throughbinoculars. It is part of abinary system with a massiveB-type main-sequence star (spectral type B2V) designatedHD 300934.[4] It is located roughly 3,100 parsecs (10,000 light-years) away from theSolar System, but is approaching at a heliocentricradial velocity of−11.05±0.42 km/s.

Stellar properties

[edit]

The binary HD 300933/4 is a probableVV Cephei-type star[11] with a compositespectrum similar to that ofV381 Cephei (HR 8164), but with weakeremission lines ofFe II,S II, andNi II[4] (the "II" indicates that theelements are in their singlyionized state inspectroscopic notation[12]). A detailed analysis of the pair was first conducted in 1970, which yielded anabsolute magnitude of −5.3 and −2.5 in theV band for HD 300933 and HD 300934, respectively, albeit this was calculated using a distance smaller than modern estimates, at 2,500 parsecs (8,200 light-years).[4] With an updated value of3100 pc, itsKS band absolute magnitude is gauged at −10.8.[7]

HD 300933 displaysinfrared emissions that imply the existence ofcircumstellar dust at a temperature of 600 K (327 °C; 620 °F). Despite this, the system shows no signs ofultravioletextinction orreddening, meaning that the light path from the B star does not cross thewind from the supergiant component. This is thought to be either due to aninclined orbit or an unfavorable orbital phase when it was observed in 1987.[11]

The star is thought to be among thelargest stars, though its precise size is highly uncertain; a radius of 806R can be calculated from theluminosity andeffective temperature provided by Healy et al. (2023),[8] whereas Messineo et al. (2019) gives a much smaller estimate of 462R[9] (though they use a far smaller distance of 1574 or 1585 pc, which is inconsistent with theGaia EDR3parallax of0.3216±0.0315 mas[1]).

References

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  1. ^abcdeBrown, A. G. A.; et al. (Gaia collaboration) (2021)."Gaia Early Data Release 3: Summary of the contents and survey properties".Astronomy & Astrophysics.649: A1.arXiv:2012.01533.Bibcode:2021A&A...649A...1G.doi:10.1051/0004-6361/202039657.S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source atVizieR.
  2. ^abHøg, E.; et al. (February 2000). "The Tycho-2 Catalogue of the 2.5 Million Brightest Stars".Astronomy and Astrophysics.355 (1):L27 –L30.Bibcode:2000A&A...355L..27H.
  3. ^abPantaleoni González, M.; Maíz Apellániz, J.; Barbá, R. H.; Negueruela, I. (1 January 2020)."A Catalog of Galactic Multiple Systems with a Red Supergiant and a B Star".Research Notes of the AAS.4 (1): 12.arXiv:2001.11680.Bibcode:2020RNAAS...4...12P.doi:10.3847/2515-5172/ab712b.ISSN 2515-5172.
  4. ^abcdKeenan, Philip C. (1970). "The Composite Spectrum of CPD-56°3586 and the Luminosity of its Supergiant Component".The Astrophysical Journal.162: 199.Bibcode:1970ApJ...162..199K.doi:10.1086/150646.ISSN 0004-637X.
  5. ^abCutri, Roc M.; Skrutskie, Michael F.; Van Dyk, Schuyler D.; Beichman, Charles A.; Carpenter, John M.; Chester, Thomas; Cambresy, Laurent; Evans, Tracey E.; Fowler, John W.; Gizis, John E.; Howard, Elizabeth V.; Huchra, John P.; Jarrett, Thomas H.; Kopan, Eugene L.; Kirkpatrick, J. Davy; Light, Robert M.; Marsh, Kenneth A.; McCallon, Howard L.; Schneider, Stephen E.; Stiening, Rae; Sykes, Matthew J.; Weinberg, Martin D.; Wheaton, William A.; Wheelock, Sherry L.; Zacarias, N. (2003). "VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)".CDS/ADC Collection of Electronic Catalogues.2246: II/246.Bibcode:2003yCat.2246....0C.
  6. ^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 atVizieR.
  7. ^abMunari, U; Traven, G; Masetti, N; Valisa, P; Righetti, G-L; Hambsch, F-J; Frigo, A; Čotar, K; De Silva, G M; Freeman, K C; Lewis, G F; Martell, S L; Sharma, S; Simpson, J D; Ting, Y-S; Wittenmyer, R A; Zucker, D B (6 July 2021)."The GALAH survey and symbiotic stars – I. Discovery and follow-up of 33 candidate accreting-only systems".Monthly Notices of the Royal Astronomical Society.505 (4):6121–6154.arXiv:2104.02686.doi:10.1093/mnras/stab1620.ISSN 0035-8711.
  8. ^abHealy, 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.
  9. ^abMessineo, M.; Brown, A.G.A. (2019). "K-M stars of class I candidate RSGs in Gaia DR2".VizieR On-line Data Catalog.Bibcode:2019yCat..51580020M.doi:10.26093/CDS/VIZIER.51580020.Record for this source atVizieR. Originally published inBibcode:2019AJ....158...20M.
  10. ^"HD 300933".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved29 November 2024.
  11. ^abBuss, Richard H., Jr.; Snow, Theodore P., Jr. (1988)."Hot components and circumstellar grains in M supergiant syncretic binaries".The Astrophysical Journal.335: 331.Bibcode:1988ApJ...335..331B.doi:10.1086/166931.ISSN 0004-637X.
  12. ^Phillips, Kenneth J. H. (1992).Guide to the Sun.Cambridge:Cambridge University Press. p. 92.ISBN 0-521-39788-X..
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