R85

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R85
Eso9931d.jpg
The nebula N119; R85 is the brightest of the small triangle of stars in the lower right "arm".
Credit: ESO
Observation data
Epoch J2000       Equinox J2000
Constellation Dorado
Right ascension 05h 17m 56.076s [1]
Declination −69° 16′ 03.77″ [1]
Apparent magnitude  (V)10.84 [2] (10.65 - 10.80 [3] )
Characteristics
Evolutionary stage LBV [4]
Spectral type B5 Iae [3]
Apparent magnitude  (U)10.28 [2]
Apparent magnitude  (B)10.93 [2]
Apparent magnitude  (V)10.84 [2]
Apparent magnitude  (R)10.53 [2]
Apparent magnitude  (I)10.44 [2]
Apparent magnitude  (J)10.103 [1]
Apparent magnitude  (H)9.980 [1]
Apparent magnitude  (K)9.822 [1]
U−B color index −0.65 [2]
B−V color index +0.09 [2]
Variable type LBV [4]
Astrometry
Radial velocity (Rv)292 [5]  km/s
Proper motion (μ)RA: −1.0 [6]   mas/yr
Dec.: −2.3 [6]   mas/yr
Distance 160,000  ly
(50,000 [7]   pc)
Absolute magnitude  (MV)−8.2 –−8.5 [3]
Details
1960 (minimum)
Radius 135 [8]   R☉
Luminosity 350,000 [3]   L☉
Temperature 13,500 [3]   K
1983 - 1990 (maximum)
Luminosity315,000 [3]   L☉
Temperature 10,000 [3]   K
Other designations
HD  269321, CPD−69°352, 2MASS  J05175607-6916037, GSC  09162-00359, Sk−69°92
Database references
SIMBAD data

R85 (or RMC 85, after the Radcliffe Observatory Magellanic Clouds catalog [5] ) is a candidate luminous blue variable [9] located in the LH-41 OB association [10] in the Large Magellanic Cloud.

A visual band light curve for R85, plotted from ASAS-SN data R85LightCurve.png
A visual band light curve for R85, plotted from ASAS-SN data

R85 has been shown to vary erratically in brightness with an amplitude of about 0.3 magnitudes. It shows variations on several timescales, sometimes with a distinct 400 day period. It has also shown temperature changes associated with brightness changes over several years, a characteristic of luminous blue variables. [12]

Based on R85's current properties and evolutionary models, it probably started out with an initial mass of 28  M☉. [10] It is theorized to be making a bubble known as DEM L132a with its stellar wind in the nebula LHA-120 N119, along with S Doradus. [13] It has an infrared excess consistent with a stellar wind contribution. [4]

Related Research Articles

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<span class="mw-page-title-main">Luminous blue variable</span> Type of star that is luminous, blue, and variable in brightenss

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<span class="mw-page-title-main">P Cygni</span> Variable star in the constellation Cygnus

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<span class="mw-page-title-main">HD 5980</span> Triple star system in the constellation Tucana

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<span class="mw-page-title-main">SMC 018136</span> Star in the Small Magellanic Cloud in the constellation Tucana

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References

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  2. 1 2 3 4 5 6 7 8 Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues. 2237. Bibcode:2002yCat.2237....0D.
  3. 1 2 3 4 5 6 7 Van Genderen, A. M. (2001). "S Doradus variables in the Galaxy and the Magellanic Clouds". Astronomy and Astrophysics. 366 (2): 508–531. Bibcode:2001A&A...366..508V. CiteSeerX   10.1.1.459.5400 . doi:10.1051/0004-6361:20000022. S2CID   55796300.
  4. 1 2 3 Bonanos, A. Z.; Massa, D. L.; Sewilo, M.; Lennon, D. J.; Panagia, N.; Smith, L. J.; Meixner, M.; Babler, B. L.; Bracker, S.; Meade, M. R.; Gordon, K. D.; Hora, J. L.; Indebetouw, R.; Whitney, B. A. (2009). "Spitzersage Infrared Photometry of Massive Stars in the Large Magellanic Cloud". The Astronomical Journal. 138 (4): 1003–1021. arXiv: 0905.1328 . Bibcode:2009AJ....138.1003B. doi:10.1088/0004-6256/138/4/1003. S2CID   14056495.
  5. 1 2 Feast, M. W.; Thackeray, A. D.; Wesselink, A. J. (1960). "The brightest stars in the Magellanic Clouds". Monthly Notices of the Royal Astronomical Society. 121 (4): 337. Bibcode:1960MNRAS.121..337F. doi: 10.1093/mnras/121.4.337 .
  6. 1 2 Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27. Bibcode:2000A&A...355L..27H.
  7. ↑ Aldoretta, E. J.; Caballero-Nieves, S. M.; Gies, D. R.; Nelan, E. P.; Wallace, D. J.; Hartkopf, W. I.; Henry, T. J.; Jao, W.-C.; Maíz Apellániz, J.; Mason, B. D.; Moffat, A. F. J.; Norris, R. P.; Richardson, N. D.; Williams, S. J. (2015). "The Multiplicity of Massive Stars: A High Angular Resolution Survey with the Guidance Sensor". The Astronomical Journal. 149 (1): 26. arXiv: 1410.0021 . Bibcode:2015AJ....149...26A. doi:10.1088/0004-6256/149/1/26. S2CID   58911264.
  8. ↑ Stahl, O.; Wolf, B.; Leitherer, C.; Zickgraf, F.-J.; Krautter, J.; De Groot, M. (1984). "Variable blue supergiants in the Large Magellanic Cloud - R 84, R 85, and R 99". Astronomy and Astrophysics. 140: 459. Bibcode:1984A&A...140..459S.
  9. ↑ Richardson, Noel D.; Mehner, Andrea (2018). "The 2018 Census of Luminous Blue Variables in the Local Group". Research Notes of the American Astronomical Society. 2 (3): 121. arXiv: 1807.04262 . Bibcode:2018RNAAS...2..121R. doi:10.3847/2515-5172/aad1f3. S2CID   119509358.
  10. 1 2 Smith, Nathan; Tombleson, Ryan (2015). "Luminous blue variables are antisocial: Their isolation implies that they are kicked mass gainers in binary evolution". Monthly Notices of the Royal Astronomical Society. 447 (1): 598–617. arXiv: 1406.7431 . Bibcode:2015MNRAS.447..598S. doi:10.1093/mnras/stu2430. S2CID   119284620.
  11. ↑ "ASAS-SN Variable Stars Database". ASAS-SN Variable Stars Database. ASAS-SN. Retrieved 6 January 2022.
  12. ↑ Van Genderen, A. M.; Sterken, C.; De Groot, M. (1998). "Light variations of massive stars (alpha Cyg variables). XVI. The LMC supergiants R 85 (LBV) and R 110 (LBV) and the SMC supergiants R 42 and R 45". Astronomy and Astrophysics. 337: 393. Bibcode:1998A&A...337..393V.
  13. ↑ Ambrocio-Cruz, P.; Rosado, M.; Laval, A.; Le Coarer, E.; Russeil, D.; Amram, P. (2008). "Kinematic field of the S-shaped nebula N119 in the LMC". Revista Mexicana de Astronomía y Astrofísica. 44: 355. Bibcode:2008RMxAA..44..355A.
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