Star in the constellation of Columba
WZ Columbae , also known asHD 38170 , is a solitary,[ 19] bluish-white huedstar located in the southernconstellation Columba , the dove. It has anapparent magnitude of 5.28,[ 3] allowing it to be faintly visible to thenaked eye . Based onparallax measurements from theGaia spacecraft , the object is about 365light years distant.[ 2] It appears to be receding from theSolar System , having a heliocentricradial velocity of 36.3 km/s .[ 9]
The star was discovered to be avariable star when theHipparcos data was analyzed. It was given itsvariable star designation in 1999.[ 20] WZ Columbae was originally listed as aslowly pulsating B-type star by theGeneral Catalogue of Variable Stars . However, observations from Hempel & Howlger (2003) reveal it to be overabundant instrontium andbarium .[ 14] Combined with Hipparcos photometry, this led to the object being reclassified as anAlpha2 Canum Venaticorum variable .[ 8] Based on data collected in theHipparcos passband , it fluctuates betweenmagnitudes 5.27 and 5.29 over 1.38days .[ 7] [ 21] However,TESS data suggests a period of 2.76618± 0.00004 days; double that of the earlier data.[ 16]
Thestellar classification of WZ Columbae is B9/9.5 V[ 5] — amain-sequence star with the characteristics of a B9 and B9.5 star. It has 3.07[ 4] times themass of the Sun and is estimated to be 394million years old,[ 16] having completed 89.2% of itsmain sequence lifetime.[ 4] It has a slightly enlargedradius of 3.47 R ☉ [ 11] and aneffective temperature of 10,000 K .[ 4] This yields aluminosity 124 times that of theSun [ 12] from itsphotosphere . Like mostchemically peculiar stars , WZ Columbae has a relatively slowprojected rotational velocity at 65 km/s .[ 15]
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(9 September 2019)."The RevisedTESS Input Catalog and Candidate Target List" .The Astronomical Journal .158 (4): 138.arXiv :1905.10694 .Bibcode :2019AJ....158..138S .doi :10.3847/1538-3881/ab3467 .eISSN 1538-3881 . ^a b Hempel, M.; Holweger, H. (September 2003)."Abundance analysis of late B stars" .Astronomy & Astrophysics .408 (3):1065– 1076.Bibcode :2003A&A...408.1065H .doi :10.1051/0004-6361:20030889 .eISSN 1432-0746 .ISSN 0004-6361 . ^a b Royer, F.; Gerbaldi, M.; Faraggiana, R.; Gómez, A. E. (January 2002)."Rotational velocities of A-type stars" .Astronomy & Astrophysics .381 (1):105– 121.arXiv :astro-ph/0110490 .Bibcode :2002A&A...381..105R .doi :10.1051/0004-6361:20011422 .eISSN 1432-0746 .ISSN 0004-6361 . ^a b c David-Uraz, A; Shultz, M E; Petit, V; Bowman, D M; Erba, C; Fine, R A; Neiner, C; Pablo, H; Sikora, J; ud-Doula, A; Wade, G A (1 April 2021)."MOBSTER – IV. 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