NSV 11749: Symbiotic nova, not a born-again red giant

Howard E. Bond, Mansi M. Kasliwal

Research output: Contribution to journalArticlepeer-review

7 Scopus citations

Abstract

NSV 11749 is a little-studied variable star, discovered by W. J. Luyten, which had a long-duration outburst around the year 1903, reaching blue magnitude 12.5 at maximum. Following the outburst, it has apparently been quiescent at about blue magnitude 17 for the past century. It was recently suggested that NSV 11749 may have been a low- or intermediate-mass star that underwent a final helium shell flash, making it temporarily a "born-again" red giant. If so, it would be only the fourth known member of this class, along with V605 Aql, FG Sge, and V4334 Sgr. However, our newly obtained optical and near-IR spectra of the object show that it is instead a symbiotic binary, with strong Balmer and He I-II emission lines, combined with a cool red-giant companion of spectral type M1-2 III. The 1903 outburst was most likely a symbiotic nova event, of which less than a dozen are known at present.

Original languageEnglish (US)
Pages (from-to)1262-1265
Number of pages4
JournalPublications of the Astronomical Society of the Pacific
Volume124
Issue number922
DOIs
StatePublished - Dec 2012

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

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