GW Librae: a unique laboratory for pulsations in an accreting white dwarf

GW Librae: a unique laboratory for pulsations in an accreting white dwarf

Non-radial pulsations have been identified in a number of accreting white dwarfs in cataclysmic variables. These stars offer insight into the excitation of pulsation modes in atmospheres with mixed compositions of hydrogen, helium, and metals, and the response of these modes to changes in the white...

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Bibliographic Details
Main Authors: Toloza, O., Gänsicke, B. T., Hermes, J. J., Townsley, D. M., Schreiber, M. R., Szkody, P., Pala, A., Beuermann, K., Bildsten, L., Breedt, E., Cook, M., Godon, P., Henden, A. A., Hubeny, I., Knigge, C., Long, K. S., Marsh, T. R., de Martino, D., Mukadam, A. S., Myers, G., Nelson, P., Oksanen, A., Patterson, J., Sion, E. M., Zorotovic, M.
Other Authors: Univ Arizona, Dept Astron, Steward Observ
Language:en
Published: OXFORD UNIV PRESS 2016
Subjects:
binaries: close
stars: individual: GW Librae
stars: variables: general
white dwarfs
Online Access:http://hdl.handle.net/10150/621433
http://arizona.openrepository.com/arizona/handle/10150/621433

Internet

http://hdl.handle.net/10150/621433
http://arizona.openrepository.com/arizona/handle/10150/621433

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