Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Nicola Clementel"'
Autor:
Augusto Damineli, Michael F. Corcoran, Noel D. Richardson, T. R. Gull, Thomas Madura, Gerd Weigelt, K. Hamaguchi, D. J. Hillier, A. F. J. Moffat, Nicola Clementel
Publikováno v:
Proceedings of the International Astronomical Union. 14:62-66
Eta Carinae is the most massive active binary within 10,000 light-years. While famous for the largest non-terminal stellar explosion ever recorded, observations reveal a supermassive (∼120 M⊙) binary consisting of an LBV and either a WR or extrem
Autor:
Theodore R. Gull, M. Teodoro, Michael F. Corcoran, Anthony F. J. Moffat, Jose H. Groh, Thomas I. Madura, Nicola Clementel, Frederick M. Walter, D. John Hillier, Augusto Damineli, Kenji Hamaguchi, Noel D. Richardson, Lucas St-Jean, Christopher M. P. Russell
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 461:2540-2558
We have monitored the massive binary star $\eta$ Carinae with the CTIO/SMARTS 1.5~m telescope and CHIRON spectrograph from the previous apastron passage of the system through the recent 2014.6 periastron passage. Our monitoring has resulted in a larg
Autor:
D. John Hillier, Gerd Weigelt, Kenji Hamaguchi, Thomas I. Madura, Noel D. Richardson, M. Teodoro, Theodore R. Gull, Nicola Clementel, Augusto Damineli, Keith Feggans, Michael F. Corcoran, Jose H. Groh, Anthony F. J. Moffat, Don J. Lindler
Publikováno v:
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Universidade de São Paulo (USP)
instacron:USP
Eta Carinae, the closest, active, massive binary containing a highly unstable LBV, exhibits expanding, compressed wind shells, seen in emission, that are spatially and spectrally resolved by \hst/\stis. Starting in June 2009, these structures were ma
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::53cfdfe03ef2294f5975950e9d2d4726
http://arxiv.org/abs/1608.06193
http://arxiv.org/abs/1608.06193
Autor:
R. Grellmann, Dieter Schertl, Michael F. Corcoran, Sridharan Rengaswamy, Gerd Weigelt, T. I. Madura, D. J. Hillier, Th. Rivinius, F. Patru, M. Teodoro, Markus Schöller, K. Ohnaka, M. Heininger, S. Guieu, A. Mérand, R. G. Petrov, T. R. Gull, Nicola Clementel, Karl-Heinz Hofmann, A. F. J. Moffat, Stefan Kraus, F. Millour, W. J. de Wit, J. H. Groh, Andrea Mehner, Noel D. Richardson, C. A. Hummel, Augusto Damineli, Markus Wittkowski
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2016, ⟨10.1051/0004-6361/201628832⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2016, ⟨10.1051/0004-6361/201628832⟩
International audience; Context. The mass loss from massive stars is not understood well. Eta Car is a unique object for studying the massive stellar wind during the LBV phase. It is also an eccentric binary with a period of 5.54 yr. The nature of bo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7e1398ed82b1220d3cf97bd3ced6cae2
Autor:
Theodore R. Gull, C. J. H. Kruip, Jan-Pieter Paardekooper, Thomas I. Madura, Nicola Clementel
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 447(3), 2445-2458
Monthly Notices of the Royal Astronomical Society, 447(3), 2445-2458
The highly eccentric binary system Eta Carinae shows numerous time-variable emission and absorption features. These observational signatures are the result of interactions between the complex three-dimensional (3D) wind-wind collision regions and pho
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d3e58e00494f21c3981cf45083795931
Autor:
Noel Richardson, Anthony F. J. Moffat, Gerd Weigelt, Keith Feggans, J. H. Groh, Nicola Clementel, Thomas I. Madura, Kenji Hamaguchi, Michael F. Corcoran, Mairan Teodoro, D. John Hillier, Don Lindler, Theodore R. Gull, Augusto Damineli
Publikováno v:
Proceedings of the International Astronomical Union. 12:420-420
Eta Carinae is the most massive active binary within 10,000 light-years and is famous for the largest non-terminal stellar explosion ever recorded. Observations reveal that the supermassive (~120 M⊙) binary, consisting of an LBV and either a WR or