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V 4049 Sgr

  • M. F. McCarthy
  • B. M. Lasker
  • T. D. Kinman
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 95)

Abstract

V 4049 Sgr was detected by the authors as a possible symbiotic star on Curtis Schmidt objective prism plates. This star is Nova Sgr 1978 and was first discovered by Stenholm and Lindstrom, When observed in 1979 With SIT specgrograph on CTIO 4 m telescope the outstanding features were the presence of very strong lines of [FeVII] chiefly at 6085 A where its flux relative to Hα is 1.6. Details have been published in Pub. astr. Soc. Pacific, 93, 470 (1981).

Keywords

High Velocity Publishing Company High Mass Mass Loss Rate Pulsation Period 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Copyright information

© D. Reidel Publishing Company, Dordrecht, Holland 1982

Authors and Affiliations

  • M. F. McCarthy
    • 1
  • B. M. Lasker
    • 2
  • T. D. Kinman
    • 3
  1. 1.Vatican ObservatorySCVItaly
  2. 2.CTIOLa SerenaChile
  3. 3.KPNOTucsonUSA

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