17 Camelopardalis

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17 Camelopardalis
Observation data
Epoch J2000      Equinox J2000
Constellation Camelopardalis
Right ascension 05h 30m 10.2021s[1]
Declination +63° 04′ 01.994″[1]
Apparent magnitude (V) 5.44[2]
Characteristics
Spectral type M1IIIa[3]
Variable type Variable star
Astrometry
Radial velocity (Rv) -20.76[4] km/s
Proper motion (μ) RA: -5.63[1] mas/yr
Dec.: -4.63[1] mas/yr
Parallax (π) 3.47 ± 0.27 mas
Distance 940 ± 70 ly
(290 ± 20 pc)
Absolute magnitude (MV) 0.95[5]
Other designations
NSV 2003, SAO 13518, BD+62° 759, HD 35583, FK5 203, HIP 25769, HR 1802.
Database references
SIMBAD data

17 Camelopardalis is red giant star in the constellation Camelopardalis. It is a suspected small amplitude variable.[2]

References[edit]

  1. ^ a b c d Van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics 474 (2): 653. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. 
  2. ^ a b Samus, N. N.; Durlevich, O. V.; et al. (2004). "VizieR Online Data Catalog: Combined General Catalogue of Variable Stars (Samus+ 2004)". VizieR On-line Data Catalog: II/250. Originally published in: 2004yCat.2250....0S 2250: 0. Bibcode:2004yCat.2250....0S. 
  3. ^ Kwok, Sun; Volk, Kevin; Bidelman, William P. (1997). "Classification and Identification of IRAS Sources with Low-Resolution Spectra". The Astrophysical Journal Supplement Series 112 (2): 557. Bibcode:1997ApJS..112..557K. doi:10.1086/313038. 
  4. ^ Famaey, B.; Pourbaix, D.; Frankowski, A.; Van Eck, S.; Mayor, M.; Udry, S.; Jorissen, A. (2009). "Spectroscopic binaries among Hipparcos M giants,. I. Data, orbits, and intrinsic variations". Astronomy and Astrophysics 498 (2): 627. arXiv:0901.0934. Bibcode:2009A&A...498..627F. doi:10.1051/0004-6361/200810698. 
  5. ^ Eggen, O. J. (1992). "Asymptotic giant branch stars near the sun". The Astronomical Journal 104: 275. Bibcode:1992AJ....104..275E. doi:10.1086/116239.