DOCSLIB.ORG
Explore
Sign Up
Log In
Upload
Search
Home
» Tags
» V1500 Cygni
V1500 Cygni
Contents
Permanent Superhumps in V1974 Cyg 3
CCD Photometry of Nova V1500 Cygni Twenty Years After I
Arxiv:2001.10147V1
Publications of the Astronomical Society of the Pacific 92:338-344, June 1980
FY13 High-Level Deliverables
Binary Evolution Novae, Supernovae, and X-Ray Sources
Index to JRASC Volumes 61-90 (PDF)
CCD Photometry of Nova V1500 Cygni Twenty Years After
Arxiv:2103.14369V1 [Astro-Ph.SR] 26 Mar 2021 Oti.Ato.Os Skalnat´E Pleso Obs
Arxiv:Astro-Ph/0607609V2 10 Oct 2006 Us.Ense L 17)Sgetdta Erir Near That Suggested (1977) Al
How Astronomical Objects Are Named
CCD Photometry of Nova V1974 Cygni I. Semeniuk, W. Pych, A
INES Access Guide No. 3 Classical Novae
Two Short-Term Periodicities of Nova V1974 Cygni I. Semeniuk1 , J.A
Asynchronous Polar V1500 Cyg: Orbital, Spin and Beat Periods
Nova V1974 Cygni-Results of the 1997 Campaign
Near-IR Observations of V1500 Cyg, and WISE Data
Top View
Lecture 9 Hydrogen Burning Nucleosynthesis, Classical Novae
Spettroscopia Nel Vicino Infrarosso Della Nova PSN J00150875-3912501 in NGC 55
On the Possibility of Dust Condensation in the Ejecta of Supernova 1987A (Infrared/Novae/Pulsars) R
An Ha Image of Nova V1500 Cygni Twelve Years After Outburst
Stellar Radii and Masses, Stellar Interferometry
Mathematics A
174 December 2017
AN INTRODUCTION to the NRAO Very Large Array R. M. Hjellming
The Detection of Discrete Cyclotron Emission Features in Phase-Resolved Optical Spectroscopy of V1500 Cygni
ΜΕΛΕΤΗ ΤΟΥ Light-Time Effect (LITE) ΚΑΙ ΤΗΣ ΚΙΝΗΣΗΣ ΤΗΣ ΓΡΑΜΜΗΣ ΤΩΝ ΑΨΙΔΩΝ ΣTA ΔΙΠΛΑ ΕΚΛΕΙΠΤΙΚΑ ΣΥΣΤΗΜΑΤΑ ΑΣΤΕΡΩΝ : ΤΧ Ηer, IQ Per, UX Eri
Astronomický Ústav SAV Správa O
Novae, May 2001 Variable Star of the Month Variable Star of the Month
Cal Information Center Is to Provide the Broadest Dissemination Possi
Understanding Variable Stars
The Identification of Hydrogen-Deficient Cataclysmic Variable Donor Stars,” Harrison, T
Observations of Some Unique Variable Stars at the Crimean Astrophysical Observatory
Shedding Light on the Population of Galactic Gravitational Wave Sources