The distances of the Galactic novae

Ozdonmez A., Guver T., Cabrera-Lavers A., Ak T.

Monthly Notices of the Royal Astronomical Society, cilt.461, ss.1177-1201, 2016 (SCI-Expanded) identifier identifier

  • Yayın Türü: Makale / Tam Makale
  • Cilt numarası: 461
  • Basım Tarihi: 2016
  • Doi Numarası: 10.1093/mnras/stw1362
  • Dergi Adı: Monthly Notices of the Royal Astronomical Society
  • Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Sayfa Sayıları: ss.1177-1201
  • Anahtar Kelimeler: stars: distances, novae, cataclysmic variables, RED CLUMP STARS, 0.8-2.5 MICRON SPECTROSCOPY, NEAR-INFRARED SPECTROSCOPY, EARLY SPECTRAL EVOLUTION, LARGE-MAGELLANIC-CLOUD, V4444 SAGITTARII 1999, UBV COLOR EVOLUTION, K-BAND MAGNITUDE, X-RAY-EMISSION, ABSOLUTE MAGNITUDES
  • Atatürk Üniversitesi Adresli: Hayır

Özet

Utilizing the unique location of red clump giants on colour-magnitude diagrams obtained from various near-infrared surveys, we derived specific reddening-distance relations towards 119 Galactic novae for which independent reddening measurements are available. Using the derived distance-extinction relation and the independent measurements of reddening we calculated the most likely distances for each system. We present the details of our distance measurement technique and the results of this analysis, which yielded the distances of 73 Galactic novae and allowed us to set lower limits on the distances of 46 systems. We also present the reddening-distance relations derived for each nova, which may be useful to analyse the different Galactic components present in the line of sight.