Astronomy:V744 Centauri
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Short description: Star in the constellation Centaurus
Observation data Equinox J2000.0]] (ICRS) | |
---|---|
Constellation | Centaurus |
Right ascension | 13h 39m 59.80667s[2] |
Declination | –49° 56′ 59.8395″[2] |
Apparent magnitude (V) | 5.1-6.7 |
Characteristics | |
Spectral type | M5III |
Variable type | Semiregular variable |
Astrometry | |
Radial velocity (Rv) | –10.7 km/s |
Proper motion (μ) | RA: –100.11 ± 0.24[2] mas/yr Dec.: 18.74 ± 0.29[2] mas/yr |
Parallax (π) | 6.35 ± 0.33[2] mas |
Distance | 510 ± 30 ly (157 ± 8 pc) |
Other designations | |
Database references | |
SIMBAD | data |
V744 Centauri, is a semi-regular variable pulsating star in the constellation Centaurus. Located 3 degrees north north east of Epsilon Centauri, It ranges from apparent magnitude 5.1 to 6.7 over 90 days.[3] It is unusual in that it is a red star with a high proper motion (greater than 50 milliarcseconds a year).[4]
References
- ↑ "ASAS All Star Catalogue". The All Sky Automated Survey. http://www.astrouw.edu.pl/asas/?page=aasc.
- ↑ 2.0 2.1 2.2 2.3 2.4 van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics 474 (2): 653–664. doi:10.1051/0004-6361:20078357. Bibcode: 2007A&A...474..653V. http://www.aanda.org/articles/aa/full/2007/41/aa8357-07/aa8357-07.html.Vizier catalog entry
- ↑ Simpson, Phil (2012). Guidebook to the Constellations: Telescopic Sights, Tales, and Myths. New York, New York: Springer Science & Business Media. pp. 252. ISBN 978-1-4419-6941-5. https://books.google.com/books?id=7gde2t9ta4QC&pg=PA252.
- ↑ Jiménez-Esteban, F. M.; Caballero, J. A.; Dorda, R.; Miles-Páez, P. A.; Solano, E. (2012). "Identification of red high proper-motion objects in Tycho-2 and 2MASS catalogues using Virtual Observatory tools". Astronomy & Astrophysics 539: 12. doi:10.1051/0004-6361/201118375. Bibcode: 2012A&A...539A..86J.
Original source: https://en.wikipedia.org/wiki/V744 Centauri.
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