The decline in irradiation from the white dwarf in old novae-Reference-Cited by-同舟云学术

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The decline in irradiation from the white dwarf in old novae

Published:2008-03-26 Issue:2 Volume:483 Page:547-556
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Thomas N. L.,Naylor T.,Norton A. J.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:20079163/pdf

Reference51 articles.

1. Linearized limb-darkening coefficients for use in analysis of eclipsing binary light curves

2. Bergner, Y. K., Bondarenko, S. I., Miroshnichenko, A. S., et al. 1985, Astron. Tsirk., 1374

3. Cutri, R. M., Skrutskie, M. F., van Dyk, S., et al. 2003, The IRSA 2MASS All-Sky Point Source Catalog, NASA/IPAC Infrared Science Archive

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1. Eruptive novae in symbiotic systems;Monthly Notices of the Royal Astronomical Society;2023-11-15

2. Sudden and steady orbital period changes across the classical nova eruptions of DQ Her and BT Mon;Monthly Notices of the Royal Astronomical Society;2020-01-24

3. A UV and optical study of 18 old novae with Gaia DR2 distances: mass accretion rates, physical parameters, and MMRD;Astronomy & Astrophysics;2019-02

4. THE EVOLUTION OF CATACLYSMIC VARIABLES AS REVEALED BY THEIR DONOR STARS;The Astrophysical Journal Supplement Series;2011-05-23

5. NOVAE WITH LONG-LASTING SUPERSOFT EMISSION THAT DRIVE A HIGH ACCRETION RATE;The Astronomical Journal;2010-04-01

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