HD 183144

Last updated
HD 183144
HD183144LightCurve.png
A light curve for HD 183144, plotted from TESS data [1]
Observation data
Epoch J2000       Equinox J2000
Constellation Aquila
Right ascension 19h 27m 33.90756s [2]
Declination +14° 16′ 56.9284″ [2]
Apparent magnitude  (V)6.32 [3]
Characteristics
Spectral type B4III [4]
U−B color index −0.512 [5]
B−V color index −0.068±0.005 [5]
Variable type suspected [6]
Astrometry
Radial velocity (Rv)+4.0±4.3 [7] [5]  km/s
Proper motion (μ)RA: 6.162 [2]   mas/yr
Dec.: −4.550 [2]   mas/yr
Parallax (π)2.8745 ± 0.0280  mas [2]
Distance 1,130 ± 10  ly
(348 ± 3  pc)
Absolute magnitude  (MV)−0.66 [5]
Details
Mass 5.1 [8]   M☉
Radius 5.8 [9]   R☉
Luminosity 2,676 [10]   L☉
Surface gravity (log g)3.73 [8]   cgs
Temperature 15,139 [8]   K
Metallicity [Fe/H]−0.003 [8]   dex
Rotational velocity (v sin i)200 [11]  km/s
Age 160 [12]   Myr
Other designations
BD+13°4020, HD  183144, HIP  95664, HR  7396, SAO  104862 [13]
Database references
SIMBAD data

HD 183144 is a suspected variable star in the equatorial constellation of Aquila. It is a hot giant star about 1,130 light years away.

Results from the MASCARA experiment indicate that HD 183144 is a pulsating variable star with a period of 0.3649 days, during which it varies by 0.01 magnitude in white light. [14] [15] It has a mass five times that of the Sun and, at an age of 160 million years, has already evolved away from the main sequence. It has expended to nearly six times the radius of the Sun and, with an effective temperature of 15,139  K , it has a bolometric luminosity of 2,676  L☉.

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<span class="mw-page-title-main">HD 93194</span> Star in the constellation Carina

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<span class="mw-page-title-main">SY Equulei</span> High galactic latitude β Cephei variable

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<span class="mw-page-title-main">HD 27563</span> Star in the constellation Eridanus

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References

  1. ↑ "MAST: Barbara A. Mikulski Archive for Space Telescopes". Space Telescope Science Institute. Retrieved 29 September 2022.
  2. 1 2 3 4 5 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.
  3. ↑ Crawford, D. L.; et al. (1971). "Four-color, H-beta, and UBV photometry for bright B-type stars in the northern hemisphere". The Astronomical Journal. 76: 1058. Bibcode:1971AJ.....76.1058C. doi:10.1086/111220.
  4. ↑ Lesh, Janet Rountree (December 1968). "The Kinematics of the Gould Belt: an Expanding Group?". Astrophysical Journal Supplement. 17: 371. Bibcode:1968ApJS...17..371L. doi: 10.1086/190179 .
  5. 1 2 3 4 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331. arXiv: 1108.4971 . Bibcode:2012AstL...38..331A. doi:10.1134/S1063773712050015. S2CID   119257644.
  6. ↑ Kukarkin, B. V.; et al. (1981). "Nachrichtenblatt der Vereinigung der Sternfreunde e.V. (Catalogue of suspected variable stars)". Nachrichtenblatt der Vereinigung der Sternfreunde E.V. (1981). Moscow: Academy of Sciences USSR Shternberg. Bibcode:1981NVS...C......0K.
  7. ↑ Wielen, R.; Schwan, H.; Dettbarn, C.; Lenhardt, H.; Jahreiß, H.; Jährling, R. (1999). "Sixth Catalogue of Fundamental Stars (FK6). Part I. Basic fundamental stars with direct solutions". Veroeffentlichungen des Astronomischen Rechen-Instituts Heidelberg. 35: 1. Bibcode:1999VeARI..35....1W.
  8. 1 2 3 4 Anders, F.; Khalatyan, A.; Queiroz, A. B. A.; Chiappini, C.; Ardevol, J.; Casamiquela, L.; Figueras, F.; Jimenez-Arranz, O.; Jordi, C.; Monguio, M.; Romero-Gomez, M.; Altamirano, D.; Antoja, T.; Assaad, R.; Cantat-Gaudin, T.; Castro-Ginard, A.; Enke, H.; Girardi, L.; Guiglion, G.; Khan, S.; Luri, X.; Miglio, A.; Minchev, I.; Ramos, P.; Santiago, B. X.; Steinmetz, M. (2022). "VizieR Online Data Catalog: StarHorse2, Gaia EDR3 photo-astrometric distances (Anders+, 2022)". Vizier Online Data Catalog. Bibcode:2022yCat.1354....0A.
  9. ↑ Kervella, Pierre; Arenou, Frédéric; Thévenin, Frédéric (2022). "Stellar and substellar companions from Gaia EDR3. Proper-motion anomaly and resolved common proper-motion pairs". Astronomy and Astrophysics. 657: 657. arXiv: 2109.10912 . Bibcode:2022A&A...657A...7K. doi:10.1051/0004-6361/202142146. S2CID   237605138.
  10. ↑ Fouesneau, M.; Andrae, R.; Dharmawardena, T.; Rybizki, J.; Bailer-Jones, C. A. L.; Demleitner, M. (2022). "Astrophysical parameters from Gaia DR2, 2MASS, and AllWISE". Astronomy and Astrophysics. 662: A125. arXiv: 2201.03252 . Bibcode:2022A&A...662A.125F. doi:10.1051/0004-6361/202141828. S2CID   245837778.
  11. ↑ Abt, Helmut A.; et al. (July 2002). "Rotational Velocities of B Stars". The Astrophysical Journal. 573 (1): 359–365. Bibcode:2002ApJ...573..359A. doi: 10.1086/340590 .
  12. ↑ Gontcharov, G. A. (2012). "Dependence of kinematics on the age of stars in the solar neighborhood". Astronomy Letters. 38 (12): 771–782. arXiv: 1606.08814 . Bibcode:2012AstL...38..771G. doi:10.1134/S1063773712120031. S2CID   118345778.
  13. ↑ "HD 183144". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2021-03-02.
  14. ↑ Burggraaff, O.; Talens, G. J. J.; Spronck, J.; Lesage, A. L.; Stuik, R.; Otten, G. P. P. L.; Van Eylen, V.; Pollacco, D.; Snellen, I. A. G. (September 2018). "Studying bright variable stars with the Multi-site All-Sky CAmeRA (MASCARA)". Astronomy and Astrophysics. 617: A32. arXiv: 1806.02247 . Bibcode:2018A&A...617A..32B. doi: 10.1051/0004-6361/201833142 .
  15. ↑ "NSV 12049". The International Variable Star Index. AAVSO. Retrieved 29 September 2022.
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