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Asteroseismology of a star cooled by neutrino emission: The pulsating pre-white dwarf PG 0122 + 200
M. S. O'Brien*, G. Vauclair, S. D. Kawaler, T. K. Watson, D. E. Winget, R. E. Nather, M. Montgomery, A. Nitta, S. J. Kleinman, D. J. Sullivan, X. J. Jiang, T. M.K. Marar, S. Seetha, B. N. Ashoka, J. Bhattacharya, E. M. Leibowitz, S. Hemar, P. Ibbetson, B. Warner, L. Van Zyl
*Corresponding author for this work
- Iowa State University
- Observatoire Midi-Pyrenees
- The University of Texas at Austin
- California Institute of Technology
- Victoria University of Wellington
- Chinese Academy of Sciences
- Indian Space Research Organization
- Tel Aviv University
- University of Cape Town
- Polish Academy of Sciences
- Pedagogical University of Cracow
- Jagiellonian University in Kraków
- Observatoire de Paris
- University of Tromsø – The Arctic University of Norway
- Isaac Newton Telescope
- Universidade Federal do Rio Grande do Sul
- Observatorio do Pico Dos Dias
- University of Delaware
- Florida Institute of Technology
Research output: Contribution to journal › Article › peer-review
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