HD 35619
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Auriga |
Right ascension | 05h 27m 36.1468s[1] |
Declination | +34° 45′ 18.959″[1] |
Apparent magnitude (V) | 8.572[2] |
Characteristics | |
Spectral type | O7.5V((f))z[3] |
U−B color index | -0.701[2] |
B−V color index | +0.242[2] |
Astrometry | |
Radial velocity (Rv) | -1.5[4] km/s |
Proper motion (μ) | RA: +2.5[5] mas/yr Dec.: -6.9[5] mas/yr |
Details | |
Rotational velocity (v sin i) | 39[6] km/s |
Other designations | |
Database references | |
SIMBAD | data |
Data sources: | |
Hipparcos Catalogue, CCDM (2002), Bright Star Catalogue (5th rev. ed.) |
HD 35619 is a double star[7] in the northern constellation of Auriga. It has an apparent magnitude of 8.572,[2] which is too faint to be viewed with the naked eye.
References
- 1 2 Hog, E.; Kuzmin, A.; Bastian, U.; Fabricius, C.; Kuimov, K.; Lindegren, L.; Makarov, V. V.; Roeser, S. (1998). "The TYCHO Reference Catalogue". Astronomy and Astrophysics 335: L65. Bibcode:1998A&A...335L..65H.
- 1 2 3 4 Landolt, A. U.; Blondeau, K. L. (June 1972), "UBV observations of the eclipsing binary LY Aurigae", Publications of the Astronomical Society of the Pacific 84: 394, Bibcode:1972PASP...84..394L, doi:10.1086/129301
- ↑ Sota, A.; et al. (March 2014), "The Galactic O-star spectroscopic survey (GOSSS). II. Bright southern stars", Astronomy & Astrophysics 563 (1): 84, arXiv:1312.6222, Bibcode:2014ApJS..211...10S, doi:10.1088/0067-0049/211/1/10, 10
- ↑ Evans, D. S. (June 20–24, 1966). "The Revision of the General Catalogue of Radial Velocities". In Batten, Alan Henry; Heard, John Frederick. Determination of Radial Velocities and their Applications, Proceedings from IAU Symposium no. 30. Determination of Radial Velocities and their Applications 30 (University of Toronto: International Astronomical Union). p. 57. Bibcode:1967IAUS...30...57E.
- 1 2 Høg, E.; et al. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics 355: L27. Bibcode:2000A&A...355L..27H.
- ↑ Simón-Díaz, S.; Herrero, A. (2014). "The IACOB project: I. Rotational velocities in northern Galactic O- and early B-type stars revisited. The impact of other sources of line-broadening". Astronomy & Astrophysics 562: A135. Bibcode:2014A&A...562A.135S. doi:10.1051/0004-6361/201322758.
- ↑ Mason, Brian D.; et al. (February 2009), "The High Angular Resolution Multiplicity of Massive Stars", The Astronomical Journal 137 (2): 3358−3377, Bibcode:2009AJ....137.3358M, doi:10.1088/0004-6256/137/2/3358
External links
|
This article is issued from Wikipedia - version of the Saturday, January 16, 2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.