HS 2325 + 8205 —An Ideal Laboratory for Accretion Disk Physics-Reference-Cited by-同舟云学术

HS 2325 + 8205 —An Ideal Laboratory for Accretion Disk Physics

Published:2012-03 Issue:913 Volume:124 Page:204-211
ISSN:0004-6280
Container-title:Publications of the Astronomical Society of the Pacific
language:en
Short-container-title:Publications of the Astronomical Society of the Pacific

Author:

Pyrzas S.,Gänsicke B. T.,Thorstensen J. R.,Aungwerojwit A.,Boyd D.,Brady S.,Casares J.,Hickman R. D. G.,Marsh T. R.,Miller I.,Ögmen Y.,Pietz J.,Poyner G.,Rodríguez-Gil P.,Staels B.

Publisher

IOP Publishing

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference44 articles.

1. Statistical analysis of the long-term visual light curve parameters of dwarf novae

2. HS 0139+0559, HS 0229+8016, HS 0506+7725, and HS 0642+5049: four new long-period cataclysmic variables

3. The dwarf nova Z Chamaeleontis - I. Photometry

4. On the late spectral types of cataclysmic variable secondaries

5. Using FU Orionis outbursts to constrain self-regulated protostellar disk models

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1. Nine New Cataclysmic Variable Stars with Negative Superhumps;The Astrophysical Journal;2024-02-01

2. The Z Camelopardalis-type Star AY Piscium: Stellar and Accretion Disk Parameters;The Astrophysical Journal;2023-06-01

3. First discovery of quasi-periodic oscillations in the dwarf nova HS 2325+8205 based on TESS photometry;Monthly Notices of the Royal Astronomical Society;2022-12-05

4. TESS and ZTF Observations of an Eclipsing Z Cam-type Dwarf Nova IPHAS J051814.34+294113.2;The Astronomical Journal;2021-10-20

5. Testing the disk instability model of cataclysmic variables;Astronomy & Astrophysics;2018-09