QV Normae

QV Normae, also known as Norma X-2, is a high mass X-ray binary star system in the constellation Norma. It varies between apparent magnitudes of 16.19 and 16.31.[2]

QV Normae
Observation data
Epoch J2000.0 ICRS      Equinox J2000.0 ICRS
Constellation Norma
Right ascension 15h 42m 23.36s[1]
Declination −52° 23′ 09.6″ [1]
Apparent magnitude (V) 16.19 - 16.31 [2]
Characteristics
Spectral type B0Iabe[2]
Other designations
Norma X-2
Database references
SIMBADdata

The X-ray source was first identified in the early 1970s.[3] The nature of the system was discovered in 1978 by astronomers who aligned a visual source of a reddened hot blue-white star with the X-ray source 4U 1538 - 52. The components are a blue-white supergiant estimated to have a mass around 20 times that of the Sun and a neutron star initially estimated at around 1.4 solar masses,[4] later revised to 0.8 solar masses. The stellar wind from the more massive star is drawn to the magnetic poles of neutron star, forming an accretion column and producing X-rays. The system has been estimated to lie anywhere from 4500 to 6500 parsecs (15,000-20,000 light-years) from Earth.[3]

References
  1. "V* QV Normae". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 20 May 2015.
  2. Otero, Sebastian Alberto (23 May 2011). "V QV Nor". The International Variable Star Index. Retrieved 20 May 2015.
  3. Hemphill, Paul B.; Rothschild, Richard E.; Markowitz, Alex; Fürst, Felix; Pottschmidt, Katja; Wilms, Jörn (2014). "A Clumpy Stellar Wind and Luminosity-dependent Cyclotron Line Revealed by the First Suzaku Observation of the High-mass X-Ray Binary 4U 1538-522". The Astrophysical Journal. 792 (1): 15. arXiv:1407.1028. Bibcode:2014ApJ...792...14H. doi:10.1088/0004-637X/792/1/14. S2CID 28693293.
  4. Reynolds, A. P.; Bell, S. A.; Hilditch, R. W. (1992). "Optical spectroscopy of the massive X-ray binary QV Nor (4U 1538 - 52)". Monthly Notices of the Royal Astronomical Society. 256 (4): 631–40. Bibcode:1992MNRAS.256..631R. doi:10.1093/mnras/256.4.631. ISSN 0035-8711.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.