Zobrazeno 1 - 10
of 73
pro vyhledávání: '"M. S. O'Brien"'
Autor:
Ernst Paunzen, T. K. Watson, Marek Drozdz, Z. Zemanová, Jan Janík, Gerald Handler, M. S. O’Brien, M. Rode-Paunzen
Publikováno v:
Revista Mexicana de Astronomía y Astrofísica. 56:193-199
Well-defined astrophysical constraints of white dwarfs (WDs), such as on the presence or absence of pulsational variability, are very much needed to refine and develop current models. Because these stars are rather faint and variability periods are m
Autor:
Waldemar Ogloza, P. Ibbetson, S. Zola, Matt A. Wood, M. S. O'Brien, Nicole M. Silvestri, R. E. Nather, Antonio Kanaan, E. W. Klumpe, Travis S. Metcalfe, S. Bernabei, G. Vauclair, Dong Xu, E. G. Meištas, Luciano Fraga, B. N. Ashoka, R. Kalytis, Ana Ulla, J. Krzesinski, N. Dolez, Michael D. Reed, Denis J. Sullivan, T. J. Ahrens, T. Sullivan, Rimvydas Janulis, Divas Sanwal, S. J. Kleinman, M. Chevreton, J. E. Solheim, Steven D. Kawaler, Pawel Moskalik, Roberto Silvotti, J. M. Gonzalez Perez, J. N. Fu, Xiao-Jun Jiang, Eran O. Ofek, Elia M. Leibowitz, D. Ališauskas, Anjum S. Mukadam, Gerald Handler, D. Kilkenny
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2006, 446, pp.237-257. ⟨10.1051/0004-6361:20053149⟩
Astronomy and Astrophysics-A&A, 2006, 446, pp.237-257. ⟨10.1051/0004-6361:20053149⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2006, 446, pp.237-257. ⟨10.1051/0004-6361:20053149⟩
Astronomy and Astrophysics-A&A, 2006, 446, pp.237-257. ⟨10.1051/0004-6361:20053149⟩
International audience; This paper analyses the Whole Earth Telescope observations of HL Tau 76, the first discovered pulsating DA white dwarf. The star was observed during two Whole Earth Telescope campaigns. It was a second priority target during t
Autor:
M. A. Wood, J. R. Robertson, J. C. Simpson, S. D. Kawaler, M. S. O’Brien, R. E. Nather, D. E. Winget, M. H. Montgomery, T. S. Metcalfe, X. J. Jiang, E. M. Leibowitz, P. Ibbetson, D. O’Donoghue, S. Zola, J. Krzesinski, G. Pajdosz, G. Vauclair, N. Dolez, M. Chevreton, D. J. Sullivan, A. Kanaan, A. Nitta
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, 2005, 634, pp.570-584. ⟨10.1086/496957⟩
The Astrophysical Journal, 2005, 634, pp.570-584. ⟨10.1086/496957⟩
International audience; The old nova DQ Herculis was the Whole Earth Telescope Northern Hemisphere target for the 1997 July campaign and was observed on four nights with the SARA 0.9 m telescope during 2003 June. We present updated ephemerides for th
Autor:
Chuck Claver, E. M. Potter, Timothy R. Bedding, M. Chevreton, Don Winget, Pawel Moskalik, S. J. Kleinman, Anne E. Sansom, Albert D. Grauer, Simon J. O'Toole, J. S. Dixson, Martin A. Barstow, Souza Oliveira Kepler, G. Vauclair, R. E. Nather, F. Wesemael, Z. E. Dind, M. Vuckovic, T. K. Watson, Gilles Fontaine, Paul A. Bradley, M. S. O'Brien, J. C. Clemens, Antonio Kanaan, Pierre Bergeron, J. L. Provencal, Steven D. Kawaler, N. Dolez
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2004, 428, pp.969-981. ⟨10.1051/0004-6361:20041475⟩
Astronomy and Astrophysics-A&A, 2004, 428, pp.969-981. ⟨10.1051/0004-6361:20041475⟩
International audience; We report on the analysis of multisite time-series photometry of the pulsating pre-white dwarf (GW Vir star) PG 1707+427, obtained by the Whole Earth Telescope collaboration. This is the last of the known GW Vir stars without
Autor:
N. Dolez, Pawel Moskalik, R. L. Riddle, Minia Manteiga, Gerald Handler, O. Suárez, Antonio Kanaan, W. Ogloza, J. E. Solheim, D. Kilkenny, B. N. Ashoka, Jaymie M. Matthews, Jian-Ning Fu, R. E. Nather, J. Krzesinski, M. S. O’Brien, T. J. Ahrens, Luciano Fraga, R. R. Shobbrook, Mukremin Kilic, Paul A. Bradley, Joyce A. Guzik, Eran O. Ofek, S. J. Kleinman, A. F. M. Costa, M. Müller, Nicole M. Silvestri, Elia M. Leibowitz, Margarida S. Cunha, T. K. Watson, R. Kalytis, Souza Oliveira Kepler, M. Chevreton, Fergal Mullally, O. Giovannini, Pierre Bergeron, Santosh Joshi, K. Sekiguchi, D. Ališauskas, Gilles Fontaine, E. G. Meištas, Atsuko Nitta, T. von Hippel, Divas Sanwal, Staszek Zola, D. J. Sullivan, R. Janulis, Anjum S. Mukadam, Donald E Winget, Xiao-Jun Jiang, D. W. Kurtz, Donal O'Donoghue, Roberto Silvotti, P. V. Birch, E. W. Klumpe, F. Johannessen, G. Vauclair, D. W. Xu, T. Sullivan, Matt A. Wood, P. Ibbetson, Ana Ulla, Michael D. Reed, T. S. Metcalfe, J. M. Gonzalez-Perez, S. Bernabei, Steven D. Kawaler
Publikováno v:
ResearcherID
Scopus-Elsevier
The Astrophysical Journal
The Astrophysical Journal, 2003, 594, pp.961-970. ⟨10.1086/377044⟩
Baltic Astronomy
Baltic Astronomy, 2003, 12, pp.71-103
CIÊNCIAVITAE
Repositório Institucional da UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
NASA Astrophysics Data System
Scopus-Elsevier
The Astrophysical Journal
The Astrophysical Journal, 2003, 594, pp.961-970. ⟨10.1086/377044⟩
Baltic Astronomy
Baltic Astronomy, 2003, 12, pp.71-103
CIÊNCIAVITAE
Repositório Institucional da UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
NASA Astrophysics Data System
We report our analysis of the stability of pulsation periods in the DAV star (pulsating hydrogen atmosphere white dwarf) ZZ Ceti, also called R548. On the basis of observations that span 31 years, we conclude that the period 213.13 s observed in ZZ C
Autor:
Matt A. Wood, Donald E Winget, E. W. Klumpe, R. E. Nather, Christophe Massacand, S. Hemar, T. M. K. Marar, G. Vauclair, Denis J. Sullivan, E. G. Meištas, O. Giovannini, J. Krzesinski, B. C. Bhat, Antonio Kanaan, V. C. Babu, Judith L. Provencal, P. Ibbetson, S. J. Kleinman, Paul A. Bradley, B. N. Ashoka, G. Pajdosz, E. Mashals, Staszek Zola, M. S. O’Brien, D. A. H. Buckley, H. S. Mahra, T. K. Watson, Michael H. Montgomery, Kinwah Wu, François Vuille, Elia M. Leibowitz, S. Seetha, Souza Oliveira Kepler, D. O'Donoghue, Pawel Moskalik, A. Nitta, J. E. Solheim, J. C. Clemens, S. Bard
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 314:689-701
We present a detailed mode identification performed on the 1994 Whole Earth Telescope (WET) run on GD 358. The results are compared with that obtained for the same star from the 1990 WET data. The two temporal spectra show very few qualitative differ
Autor:
M. S. O'Brien
Publikováno v:
Open Astronomy, Vol 9, Iss 1, Pp 13-22 (2000)
Autor:
M. S. O'Brien
Publikováno v:
Open Astronomy, Vol 7, Iss 1, Pp 89-98 (1998)
Autor:
P. Ibbetson, B. N. Ashoka, Pawel Moskalik, A. Nitta, T. Thomassen, O. Giovannini, J. Bhattacharya, S. Seetha, S. Hemar, S. J. Kleinman, Matt A. Wood, Denis J. Sullivan, J. E. Solheim, Judith L. Provencal, Donald E Winget, Xue-Jian Jiang, T. K. Watson, Jurek Krzesinski, J. C. Clemens, L. van Zyl, M. S. O'Brien, R. E. Nather, T. M. K. Marar, G. Vauclair, Brian Warner, Staszek Zola, G. Pajdosz, Souza Oliveira Kepler, S. D. Kawaler, Elia M. Leibowitz, M. Chevreton, N. Dolez, Michael H. Montgomery
Publikováno v:
The Astrophysical Journal. 495:458-467
Observation of g-mode pulsations in the variable pre-white dwarf (GW Virginis) stars provides a unique means to probe their interiors and to study the late stages of stellar evolution. Multisite campaigns have in several cases proved highly successfu
Autor:
M. S. O'Brien
Publikováno v:
Open Astronomy, Vol 4, Iss 3, Pp 349-354 (1995)