Spectroscopic observations of PU Vulpeculae in the 3210 - 10 950 A range during the nebular phase
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/271/4/875/2907944/mnras271-0875.pdf
Cited by 9 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. White dwarfs with planetary remnants in the era of Gaia – I. Six emission line systems;Monthly Notices of the Royal Astronomical Society;2021-04-10
2. Identification of new Galactic symbiotic stars with SALT – I. Initial discoveries and other emission line objects★;Monthly Notices of the Royal Astronomical Society;2014-03
3. EVOLUTION OF THE SYMBIOTIC NOVA PU VUL—OUTBURSTING WHITE DWARF, NEBULAE, AND PULSATING RED GIANT COMPANION;The Astrophysical Journal;2012-04-06
4. A LIGHT-CURVE MODEL OF THE SYMBIOTIC NOVA PU Vul (1979): A VERY QUIET EXPLOSION WITH LONG-LASTING FLAT PEAK;The Astrophysical Journal;2011-01-04
5. Analysis of archive UV observations of the symbiotic nova PU Vul during its nebular stage and brightness minimum in 1993–1994;Astronomy Reports;2009-11
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