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Makale Tam Makale Uluslararası 2016

The distances of the Galactic novae

Aykut Özdönmez, Tolga Guver, Antonio Cabrera-Lavers, Tansel Ak

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY Cilt 461 · ss. 1177–1201 · 11.09.2016
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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.

Anahtar kelimeler

novae cataclysmic variables stars: distances 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

Atıf için künye

Özdönmez, A., Guver, T., Cabrera-Lavers, A., & Ak, T. (2016). The distances of the Galactic novae. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 461, 1177–1201. https://doi.org/10.1093/mnras/stw1362

BibTeX 
@article{ozdonmez2016-78980,
  author = {Özdönmez, Aykut and Guver, Tolga and Cabrera-Lavers, Antonio and Ak, Tansel},
  title = {The distances of the Galactic novae},
  journal = {MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY},
  year = {2016},
  volume = {461},
  pages = {1177--1201},
  issn = {0035-8711},
  doi = {10.1093/mnras/stw1362},
  url = {https://akademik.atauni.edu.tr/yayinlar/78980-the-distances-of-the-galactic-novae}
}