Jump to content

V385 Andromedae

From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by Lithopsian (talk | contribs) at 17:50, 8 February 2016 (removed Category:M-type stars; added Category:M-type giants using HotCat). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

V385 Andromedae
Observation data
Epoch J2000      Equinox J2000
Constellation Andromeda
Right ascension 23h 24m 08.868s[1]
Declination +41° 36′ 46.35″[1]
Apparent magnitude (V) 6.424
Characteristics
Spectral type M0
B−V color index 1.702
Variable type irregular
Astrometry
Proper motion (μ) RA: -12.02 ± 0.31[1] mas/yr
Dec.: 2.46 ± 0.29[1] mas/yr
Parallax (π)3.41 ± 0.47 mas[1]
Distanceapprox. 1,000 ly
(approx. 290 pc)
Other designations
HD 220524, BD+40° 5065, HIP 115530, SAO 52978.
Database references
SIMBADdata

V385 Andromedae is a star in the constellation Andromeda. It was idenitifed as being a long-period variable in 1999.[2]

References

  1. ^ a b c d e van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357.Vizier catalog entry
  2. ^ Kazarovets, E. V.; Samus, N. N.; Durlevich, O. V.; Frolov, M. S.; Antipin, S. V.; Kireeva, N. N.; Pastukhova, E. N. (1999). "The 74th Special Name-list of Variable Stars". Information Bulletin on Variable Stars (4659). Bibcode:1999IBVS.4659....1K.{{cite journal}}: CS1 maint: multiple names: authors list (link)