The 2016-2017 peak luminosity of the pre-main sequence variable V2492 Cygni
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DOI: 10.1051/0004-6361/201731611
Abstract: Context. V2492 Cyg is a young pre-main sequence star presenting repetitive brightness variations of significant amplitude (R - 5 mag) whose physical origin has been ascribed to both extinction (UXor-type) and accretion (EXor-type) variability, although… read more here.
Keywords: pre main; v2492; accretion; main sequence ... See more keywords