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AG Pegasi
A Hot Subdwarf-White Dwarf Super-Chandrasekhar Candidate
Správa O Činnosti Organizácie SAV Za Rok 2017
National Radio Astronomy Observatory Quarterly
RESEARCH PROGRAMS 140-Foot Telescope
Appendix: Spectroscopy of Variable Stars
Observational Cosmology - 30H Course 218.163.109.230 Et Al
AG€Pegasi – Now a Classical Symbiotic Star in Outburst?
On the Study of Atomic and Molecular Processes Affecting Astrophysical
Summer Solstice 1988 No
Lectures on Astronomy, Astrophysics, and Cosmology
The Formation of the Double Gaussian Line Profiles Of
Astrophysics
Meeting Abstracts
The Balmer Decrement in the Emission Spectra of Astronomical Objects
What Is AG Pegasi? AG Pegasi Is a Symbio C Binary Star, Composed of a Red the Harvard Observing Project (See Supergiant and a White Dwarf
New Outburst of the Symbiotic Nova AG Pegasi After 165 Yr? A
The Nature of Ultraviolet Spectra of AG Pegasi and Other Symbiotic Stars: Locations, Origins, and Excitation Mechanisms of Emission Lines
Analysis of the Symbiotic Star Ag Pegasi
Top View
An Atlas of Stellar Spectra
Annual Report 2015-2016
Space Research in Slovakia 2016 - 2017
Bibliography of Lick Observatory-Based Research Publications: 2000–2011.5
Arl EPCA Report
Kevin Gah-Jan Tsang
The Hubble Catalog of Variables (HCV)? A
Journal of the Korean Society
1993Aj 106.1573K the Astronomical Journal
The Visual Line Spectrum of AG Pegasi in 1995 N.A
Observations Magnetic Tape Version R
Optical Observatories
ANALYSIS of the SYMBIOTIC STAR AG PEGASI ' Charles D. Keyes And
Symbiotic Star AG Pegasi Observed After Ourburst 1 October 2018, by Tomasz Nowakowski
Jul 2 4 1985 Table of Contents
Publication/Citation List
IN CONJUNCTION WITH: with High Energy Astrophysics Division (HEAD) and Historical Astronomy Division (HAD)
The Messenger
Ultraviolet Spectroscopy of Old Novae and Symbiotic