Astronomy:HD 33632

From HandWiki
Short description: Star in Auriga
HD 33632
Observation data
Equinox J2000.0]] (ICRS)
Constellation Auriga[1]
Right ascension  05h 13m 17.448s[2]
Declination +37° 20′ 14.32″[2]
Apparent magnitude (V) 6.47[3]
Characteristics
Evolutionary stage main sequence[2] + brown dwarf[4]
Spectral type F8V[5]
Astrometry
Proper motion (μ) RA: −133.922[2] mas/yr
Dec.: −136.772[2] mas/yr
Parallax (π)37.8953 ± 0.0263[2] mas
Distance86.07 ± 0.06 ly
(26.39 ± 0.02 pc)
Absolute magnitude (MV)+4.40[1]
Details
Aa
Mass1.14[6] M☉
Radius1.11[6] R☉
Luminosity1.51[6] L☉
Surface gravity (log g)4.40[6] cgs
Temperature6,074[6] K
Age4.8[7] Gyr
Ab
Mass46±8 MJup
Radius0.97 RJup
Other designations
BD+37°1091, HD 33632, HIP 24332, WDS J05133+3720A[8]
Database references
SIMBADdata

HD 33632 is an F-type main-sequence star with a brown dwarf companion located in the constellation of Auriga. The brown dwarf was directly imaged in mid 2024.[4]

Brown dwarf

HD 33632 Ab has a radius of 0.97 Jupiter radii[4] and a mass of 46±8 Jupiter masses.[9]

References

  1. ↑ 1.0 1.1 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode: 2012AstL...38..331A  XHIP record for this object at VizieR.
  2. ↑ 2.0 2.1 2.2 2.3 2.4 2.5 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940  Gaia DR3 record for this source at VizieR.
  3. ↑ Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P. et al. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics 355. Bibcode: 2000A&A...355L..27H. 
  4. ↑ 4.0 4.1 4.2 Morsy, Mona El; Currie, Thayne; Bovie, Danielle; Kuzuhara, Masayuki; Lacy, Brianna; Li, Yiting; Tobin, Taylor; Brandt, Timothy et al. (2025-04-03), "Dynamical and Atmospheric Characterization of the Substellar Companion HD 33632 Ab from Direct Imaging, Astrometry, and Radial-Velocity Data", The Astrophysical Journal 981 (1): 20, doi:10.3847/1538-4357/ada3be, Bibcode: 2025ApJ...981...20E 
  5. ↑ Gray, R. O.; Corbally, C. J.; Garrison, R. F.; McFadden, M. T.; Robinson, P. E. (2003). "Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 Parsecs: The Northern Sample. I.". The Astronomical Journal 126 (4): 2048. doi:10.1086/378365. Bibcode: 2003AJ....126.2048G. 
  6. ↑ 6.0 6.1 6.2 6.3 6.4 Stassun, Keivan G. et al. (2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal 158 (4): 138. doi:10.3847/1538-3881/ab3467. Bibcode: 2019AJ....158..138S. 
  7. ↑ Aguilera-Gómez, Claudia; Ramírez, Iván; Chanamé, Julio (2018). "Lithium abundance patterns of late-F stars: An in-depth analysis of the lithium desert". Astronomy and Astrophysics 614: A55. doi:10.1051/0004-6361/201732209. Bibcode: 2018A&A...614A..55A. 
  8. ↑ "HD 33632". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+33632. 
  9. ↑ Hsu, Chih-Chun; Wang, Jason J.; Xuan, Jerry W.; Ruffio, Jean-Baptiste; Morris, Evan; Echeverri, Daniel; Xin, Yinzi; Liberman, Joshua et al. (August 2024). "Rotation and Abundances of the Benchmark Brown Dwarf HD 33632 Ab from Keck/KPIC High-resolution Spectroscopy" (in en). The Astrophysical Journal 971 (1): 9. doi:10.3847/1538-4357/ad58d3. ISSN 0004-637X. Bibcode: 2024ApJ...971....9H.