Raman‐scattered Heiiλ6545 Line in the Symbiotic Star V1016 Cygni
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/598/i=1/a=553/pdf
Reference40 articles.
1. Arrieta, A. & Torres-Peimbert, S. 2000, in ASP Conf. Ser. 199, Asymmetrical Planetary Nebulae II: From Origins to Microstructures, ed. J. H. Kastner, N. Soker, & S. Rappaport (San Francisco: ASP), 255
2. Broad Hα Wings in Nebulae around Evolved Stars and in Young Planetary Nebulae
3. M2-9 - A planetary nebula with an eruptive nucleus?
4. Near-simultaneous Observations of Direct and Raman-scattered Linesin the Symbiotic Star Z Andromedae
5. Contemporaneous Ultraviolet and Optical Observations of Direct and Raman‐scattered OviLines in Symbiotic Stars
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3. MASS-LOSS RATE BY THE MIRA IN THE SYMBIOTIC BINARY V1016 CYGNI FROM RAMAN SCATTERING;The Astrophysical Journal;2015-10-21
4. Raman-Scattered HeII 1025 Line in The Symbiotic Binary V1016 Cyg As a Diagnostic Tool of The Wind From Its Mira-Type Donor;EAS Publications Series;2015
5. The spectral energy distribution of D-type symbiotic stars: the role of dust shells;Monthly Notices of the Royal Astronomical Society;2010-03-01
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