Astrometric binary in Camelopardalis.
HD 32356 , also designated as HR 1624 , is an astrometric binary located in the northern circumpolar constellation Camelopardalis , the giraffe, near β Camelopardalis . The visible component is faintly visible to the naked eye as an orange-hued star with an apparent magnitude of 5.99. Gaia DR3 parallax measurements imply a distance of 557 light-years and it is currently drifting closer with a heliocentric radial velocity of −45.2 km/s . At its current distance, HD 32356's brightness is diminished by an interstellar extinction of 0.29 magnitudes and it has an absolute magnitude of +0.23.
The visible component has a stellar classification of K5 II, indicating that it is an evolved K-type bright giant that has ceased hydrogen fusion at its core and left the main sequence . It has 1.18 times the mass of the Sun but at the age of 4.27 billion years , it has expanded to 30.67 times the radius of the Sun . It radiates 300 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,111 K . HD 32356 A is metal deficient with an iron abundance roughly half of the Sun 's and it spins too slowly for its projected rotational velocity to be measured accurately.
References
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Gaia DR3 record for this source at VizieR .
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^ Anders, F.; et al. (August 2019). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18" . Astronomy & Astrophysics . 628 : A94. arXiv :1904.11302 . Bibcode :2019A&A...628A..94A . doi :10.1051/0004-6361/201935765 . eISSN 1432-0746 . ISSN 0004-6361 . S2CID 131780028 .
^ Kervella, P.; Thévenin, F.; Di Folco, E.; Ségransan, D. (April 8, 2004). "The angular sizes of dwarf stars and subgiants: Surface brightness relations calibrated by interferometry" . Astronomy & Astrophysics . 426 (1): 297–307. arXiv :astro-ph/0404180 . Bibcode :2004A&A...426..297K . doi :10.1051/0004-6361:20035930 . eISSN 1432-0746 . ISSN 0004-6361 . S2CID 6077801 .
^ Feuillet, Diane K.; Bovy, Jo; Holtzman, Jon; Girardi, Léo; MacDonald, Nick; Majewski, Steven R.; Nidever, David L. (20 January 2016). "Determining Ages of APOGEE Giants with Known Distances" . The Astrophysical Journal . 817 (1): 40. arXiv :1511.04088 . Bibcode :2016ApJ...817...40F . doi :10.3847/0004-637X/817/1/40 . eISSN 1538-4357 . S2CID 118675933 .
^ Wu, Yue; Singh, H. P.; Prugniel, P.; Gupta, R.; Koleva, M. (2 December 2010). "Coudé-feed stellar spectral library – atmospheric parameters" . Astronomy & Astrophysics . 525 : A71. arXiv :1009.1491 . Bibcode :2011A&A...525A..71W . doi :10.1051/0004-6361/201015014 . eISSN 1432-0746 . ISSN 0004-6361 .
^ de Medeiros, J. R.; Mayor, M. (November 1999). "A catalog of rotational and radial velocities for evolved stars" . Astronomy and Astrophysics Supplement Series . 139 (3): 433–460. Bibcode :1999A&AS..139..433D . doi :10.1051/aas:1999401 . ISSN 0365-0138 . S2CID 54046583 .
"HD 32356" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved May 7, 2024.
Frankowski, A.; Jancart, S.; Jorissen, A. (19 December 2006). "Proper-motion binaries in the Hipparcos catalogue: Comparison with radial velocity data" . Astronomy & Astrophysics . 464 (1): 377–392. arXiv :astro-ph/0612449 . Bibcode :2007A&A...464..377F . doi :10.1051/0004-6361:20065526 . eISSN 1432-0746 . ISSN 0004-6361 . S2CID 14010423 .
Gontcharov, George A.; Mosenkov, Aleksandr V. (28 September 2017). "Verifying reddening and extinction for Gaia DR1 TGAS main sequence stars" . Monthly Notices of the Royal Astronomical Society . 472 (4): 3805–3820. arXiv :1709.01160 . Bibcode :2017MNRAS.472.3805G . doi :10.1093/mnras/stx2219 . eISSN 1365-2966 . ISSN 0035-8711 . S2CID 118879856 .
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