16 Puppis
Star in the constellation Puppis
16 Puppis is a suspected astrometric binary star system in the southern constellation of Puppis , and is located in the northernmost part of its constellation, almost due north of the bright star Rho Puppis , and east of Canis Major . It is visible to the naked eye as a faint, blue-white hued star with an apparent visual magnitude of 4.40. The star is located is approximately 465 light years away from the Sun based on parallax . It was the brightest star in Officina Typographica , an obsolete constellation.
The visible member is a B-type main-sequence star with a stellar classification of B5 V, according to N. Houk and M. Smith-Moore (1978). Earlier, Hoffleit et al. (1964) had listed a class of B5 IV, suggesting a more evolved subgiant star . It is spinning rapidly, which is creating an equatorial bulge that is 6% larger than the polar radius. The star is radiating 836 times the luminosity of the Sun from its photosphere at an effective temperature of 16,680 K.
References
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1 2 Houk, Nancy; Smith-Moore, M. (1978). Michigan Catalogue of Two-dimensional Spectral Types for the HD Stars . Vol. 4. Ann Arbor: Dept. of Astronomy, University of Michigan. Bibcode :1988mcts.book.....H .
1 2 Hoffleit, D.; Warren, W. H. (1995). "VizieR Online Data Catalog: Bright Star Catalogue, 5th Revised Ed. (Hoffleit+, 1991)". VizieR On-line Data Catalog: V/50. Originally Published in: 1964BS....C......0H . 5050 . Bibcode :1995yCat.5050....0H .
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↑ Abt, Helmut A.; Levato, Hugo; Grosso, Monica (2002). "Rotational Velocities of B Stars" . The Astrophysical Journal . 573 (1): 359– 365. Bibcode :2002ApJ...573..359A . doi :10.1086/340590 .
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↑ Eggleton, P. P.; Tokovinin, A. A. (September 2008). "A catalogue of multiplicity among bright stellar systems" . Monthly Notices of the Royal Astronomical Society . 389 (2): 869– 879. arXiv :0806.2878 . Bibcode :2008MNRAS.389..869E . doi :10.1111/j.1365-2966.2008.13596.x . S2CID 14878976 .
↑ Ian Ridpath's Star Tales - Officina Typographica