Search Results - "Webbink, Ronald F."

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  1. 1

    ADIABATIC MASS LOSS IN BINARY STARS. II. FROM ZERO-AGE MAIN SEQUENCE TO THE BASE OF THE GIANT BRANCH by Ge, Hongwei, Webbink, Ronald F., Chen, Xuefei, Han, Zhanwen

    Published in The Astrophysical journal (10-10-2015)
    “…ABSTRACT In the limit of extremely rapid mass transfer, the response of a donor star in an interacting binary becomes asymptotically one of adiabatic…”
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    Journal Article
  2. 2

    The Common Envelope Evolution Outcome. II. Short-orbital-period Hot Subdwarf B Binaries Reveal a Clear Picture by Ge, Hongwei, Tout, Christopher A, Webbink, Ronald F, Chen, Xuefei, Sarkar, Arnab, Li, Jiao, Li, Zhenwei, Zhang, Lifu, Han, Zhanwen

    Published in The Astrophysical journal (01-02-2024)
    “…Common envelope evolution (CEE) is vital for forming short-orbital-period compact binaries. It covers many objects, such as double compact merging binaries,…”
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  3. 3

    Adiabatic Mass Loss in Binary Stars. III. From the Base of the Red Giant Branch to the Tip of the Asymptotic Giant Branch by Ge, Hongwei, Webbink, Ronald F, Chen, Xuefei, Han, Zhanwen

    Published in The Astrophysical journal (01-08-2020)
    “…The distinguishing feature of the evolution of close binary stars is the role played by the mass exchange between the component stars. Whether or not the mass…”
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  4. 4

    Adiabatic Mass Loss in Binary Stars. I. Computational Method by Ge, Hongwei, Hjellming, Michael S, Webbink, Ronald F, Chen, Xuefei, Han, Zhanwen

    Published in The Astrophysical journal (10-07-2010)
    “…The asymptotic response of donor stars in interacting binary systems to very rapid mass loss is characterized by adiabatic expansion throughout their…”
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  5. 5

    A Catalog and Atlas of Cataclysmic Variables: The Living Edition by Downes, Ronald A., Webbink, Ronald F., Shara, Michael M., Ritter, Hans, Kolb, Ulrich, Duerbeck, Hilmar W.

    “…The Catalog and Atlas of Cataclysmic Variables (Edition 1: Downes & Shara; Edition 2: Downes, Webbink, & Shara) has been a valuable source of information for…”
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  6. 6

    Stellar adiabatic mass loss model and applications by Ge, Hongwei, Webbink, Ronald F., Han, Zhanwen, Chen, Xuefei

    Published in Astrophysics and space science (01-10-2010)
    “…Roche-lobe overflow and common envelope evolution are very important in binary evolution, which is believed to be the main evolutionary channel to hot subdwarf…”
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    A Catalog and Atlas of Cataclysmic Variables—2nd Edition by Downes, Ronald A., Webbink, Ronald F., Shara, Michael M.

    “…We present a catalog of all 1020 known cataclysmic variables (CVs). This paper is a major update of the first edition of the catalog (Downes and Shara, 1993,…”
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  10. 10

    The thermal equilibrium mass loss model and its applications in binary evolution by Ge, Hongwei, Webbink, Ronald F, Han, Zhanwen

    Published 01-06-2020
    “…Binary evolution is indispensable in stellar evolution to understand the formation and evolution of most peculiar and energetic objects, such as binary compact…”
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  11. 11

    Outbursts of the recurrent nova T Coronae Borealis by WEBBINK, RONALD F

    Published in Nature (London) (22-07-1976)
    “…The behavior of the recurrent nova T CrB is interpreted in terms of accretion in a binary system. Brightness variations in this system immediately surrounding…”
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  12. 12

    The Common Envelope Evolution Outcome. II. Short Orbital Period Hot Subdwarf B Binaries Reveal a Clear Picture by Ge, Hongwei, Tout, Christopher A, Webbink, Ronald F, Chen, Xuefei, Sarkar, Arnab, Li, Jiao, Li, Zhenwei, Zhang, Lifu, Han, Zhanwen

    Published 28-11-2023
    “…The common envelope evolution (CEE) is vital in forming short orbital period compact binaries. It covers many objects, such as double compact merging binaries,…”
    Get full text
    Journal Article
  13. 13

    Adiabatic mass loss in binary stars. III. From the base of the red giant branch to the tip of asymptotic giant branch by Ge, Hongwei, Webbink, Ronald F, Chen, Xuefei, Han, Zhanwen

    Published 20-07-2020
    “…The distinguishing feature of the evolution of close binary stars is the role played by the mass exchange between the component stars. Whether the mass…”
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    Journal Article
  14. 14

    Common Envelope Evolution of Massive Stars by Ricker, Paul M, Timmes, Frank X, Taam, Ronald E, Webbink, Ronald F

    Published 08-11-2018
    “…Proc. IAU 14 (2018) 449-454 The discovery via gravitational waves of binary black hole systems with total masses greater than $60M_\odot$ has raised…”
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  15. 15

    Watch This Space: Observing Merging White Dwarfs by Webbink, Ronald F

    Published 29-11-2010
    “…The Laser Interferometer Space Antenna (LISA) will open the low-frequency (0.1-100 mHz) part of the gravitational wave spectrum to direct observation. Of order…”
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  16. 16

    MODEST-1: Integrating stellar evolution and stellar dynamics by Hut, Piet, Shara, Michael M., Aarseth, Sverre J., Klessen, Ralf S., Lombardi Jr, James C., Makino, Junichiro, McMillan, Steve, Pols, Onno R., Teuben, Peter J., Webbink, Ronald F.

    Published in New astronomy (01-05-2003)
    “…We summarize the main results from MODEST-1, the first workshop on MOdeling DEnse STellar systems. Our goal is to go beyond traditional population synthesis…”
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  17. 17

    Adiabatic Mass Loss in Binary Stars. II. From Zero-Age Main Sequence to the Base of the Giant Branch by Ge, Hongwei, Webbink, Ronald F, Chen, Xuefei, Han, Zhanwen

    Published 17-07-2015
    “…In the limit of extremely rapid mass transfer, the response of a donor star in an interacting binary becomes asymptotically one of adiabatic expansion. We…”
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    Journal Article
  18. 18

    Common Envelope Evolution Redux by Webbink, Ronald F

    Published 02-04-2007
    “…Common envelopes form in dynamical time scale mass exchange, when the envelope of a donor star engulfs a much denser companion, and the core of the donor plus…”
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    Contact Binaries by Webbink, Ronald F

    Published 23-04-2003
    “…Despite being the most abundant (by space density) of interacting binary stars, W Ursae Majoris (W UMa) stars are not understood structurally. Their stellar…”
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