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17th European White Dwarf Workshop: Mass transfer dynamics in white dwarf binary systems
Dan, Marius (2010)
clipboard
mla
clipboard		 Dan M. "17th European White Dwarf Workshop: Mass transfer dynamics in white dwarf binary systems.", timms video, Universität Tübingen (2010): https://timms.uni-tuebingen.de:443/tp/UT_20100818_002_eurowd_0001. Accessed 20 Apr 2024.
apa
clipboard		 Dan, M. (2010). 17th European White Dwarf Workshop: Mass transfer dynamics in white dwarf binary systems. timms video: Universität Tübingen. Retrieved April 20, 2024 from the World Wide Web https://timms.uni-tuebingen.de:443/tp/UT_20100818_002_eurowd_0001
harvard
clipboard		 Dan, M. (2010). 17th European White Dwarf Workshop: Mass transfer dynamics in white dwarf binary systems [Online video]. 18 August. Available at: https://timms.uni-tuebingen.de:443/tp/UT_20100818_002_eurowd_0001 (Accessed: 20 April 2024).
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title: 17th European White Dwarf Workshop: Mass transfer dynamics in white dwarf binary systems
alt. title: 17th European White Dwarf Workshop - SN progenitors
creator: Dan, Marius (author)
subjects: Astronomie, Physik, Astrophysik, Workshop, White Dwarf, mass transfer dynamics, white dwarf binary systems, Marius Dan
description: 17th European White Dwarf Workshop, 16. bis 20. August 2010
abstract: Mass transfer dynamics in white dwarf binary systems (M. Dan, S. Rosswog, M. Brüggen) (School of Engineering and Science, Jacobs University Bremen, Campus Ring 1, 28759, Bremen, Germany) In the last stages of the gravitational wave driven inspiral of a white dwarf binary system mass transfer sets in. Once started, the mass transfer substantially alters the orbital evolution and may decide whether the binary suffers a rapid merger or undergoes a long-lived accretion phase in a semidetached binary. We study numerically the stability and outcome of such mass transfer phases. We carefully construct initial conditions that correspond to the onset of numerically resolvable mass transfer and we explore different mass ratios for both disk and direct impact accretion regimes. Our results show that mass transfer lasts for tens to hundred of orbits and that in the end the donor is tidally disrupted. Due to the finite numerical resolution these results need to be considered as lower limits on the duration of mass transfer. Finally, we investigate the observational signatures associated with such an event.
publisher: ZDV Universität Tübingen
contributor: ZDV Universität Tübingen (producer)
creation date: 2010-08-18
dc type: image
localtype: video
identifier: UT_20100818_002_eurowd_0001
language: eng
rights: Url: https://timmsstatic.uni-tuebingen.de/jtimms/TimmsDisclaimer.html?638492220404688285