Changes in the Period of Negative Superhumps of Type SU UMa Dwarf Novae. II. NY Her (2017 and 2020)-Reference-Cited by-同舟云学术

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Changes in the Period of Negative Superhumps of Type SU UMa Dwarf Novae. II. NY Her (2017 and 2020)

Published:2021-09 Issue:3 Volume:64 Page:293-305
ISSN:0571-7256
Container-title:Astrophysics
language:en
Short-container-title:Astrophysics

Author:

Pavlenko E. P.,Sosnovskii A. A.,Antonyuk K. A.,Antonyuk O. I.,Pit’ N. V.,Kokhirova G. I.,Rakhmatullaeva F. J.,Baklanov A. V.

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

https://link.springer.com/content/pdf/10.1007/s10511-021-09690-3.pdf

Reference30 articles.

1. B. Warner, Cataclysmic Variable Stars, Cambridge University Press (1995).

2. Y. Osaki, Publ. Astron. Soc. Pacif. 108, 39 (1996).

3. J. K. Cannizzo, Astrophys. J. 419, 318 (1993).

4. J.-P. Lasota, NewAR 45, 449 (2001).

5. R. Whitehurst, Mon. Not. Roy. Astron. Soc. 232, 35 (1988).

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2. Negative and positive superhumps of V503 Cyg as seen in TESS data. I. Seasons 2019 and 2021;Contributions of the Astronomical Observatory Skalnaté Pleso;2024-02-01

3. Accreting White Dwarfs;Handbook of X-ray and Gamma-ray Astrophysics;2024

4. Evolution of Negative Superhumps, Quasiperiodic Oscillations, and Outbursts in the Z Cam-type Dwarf Nova AH Her;The Astrophysical Journal;2023-09-26

5. Superhumps in the cataclysmic variable BG Triangulum;Monthly Notices of the Royal Astronomical Society;2022-08-22

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