The Onfp class in the Magellanic Clouds

The Onfp class of rotationally broadened, hot spectra was defined some time ago in the Galaxy, where its membership to date numbers only eight. The principal defining characteristic is a broad, centrally reversed He II λ 4686 emission profile; other emission and absorption lines are also rotationall...

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Autores principales: Walborn, Nolan Revere, Howarth, Ian D., Evans, Christopher J., Crowther, Paul A., Moffat, Anthony F. J., St-Louis, Nicole, Fariña, Cecilia, Bosch, Guillermo Luis, Morrell, Nidia Irene, Barbá, Rodolfo Héctor, Loon, Jacco T. van
Formato: Articulo
Lenguaje:Inglés
Publicado: 2010
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/82516
Aporte de:
id I19-R120-10915-82516
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
Magellanic Clouds
Stars: early-type
Stars: emission-line, Be
Stars: fundamental parameters
Stars: rotation
Stars: variables: general
spellingShingle Ciencias Astronómicas
Magellanic Clouds
Stars: early-type
Stars: emission-line, Be
Stars: fundamental parameters
Stars: rotation
Stars: variables: general
Walborn, Nolan Revere
Howarth, Ian D.
Evans, Christopher J.
Crowther, Paul A.
Moffat, Anthony F. J.
St-Louis, Nicole
Fariña, Cecilia
Bosch, Guillermo Luis
Morrell, Nidia Irene
Barbá, Rodolfo Héctor
Loon, Jacco T. van
The Onfp class in the Magellanic Clouds
topic_facet Ciencias Astronómicas
Magellanic Clouds
Stars: early-type
Stars: emission-line, Be
Stars: fundamental parameters
Stars: rotation
Stars: variables: general
description The Onfp class of rotationally broadened, hot spectra was defined some time ago in the Galaxy, where its membership to date numbers only eight. The principal defining characteristic is a broad, centrally reversed He II λ 4686 emission profile; other emission and absorption lines are also rotationally broadened. Recent surveys in the Magellanic Clouds (MCs) have brought the class membership there, including some related spectra, to 28. We present a survey of the spectral morphology and rotational velocities, as a first step toward elucidating the nature of this class. Evolved, rapidly rotating hot stars are not expected theoretically, because the stellar winds should brake the rotation. Luminosity classification of these spectra is not possible, because the principal criterion (He II λ4686) is peculiar; however, the MCs provide reliable absolute magnitudes, which show that they span the entire range from dwarfs to supergiants. The Onfp line-broadening distribution is distinct and shifted toward larger values from those of normal O dwarfs and supergiants with >99.99% confidence. All cases with multiple observations show line-profile variations, which even remove some objects from the class temporarily. Some of them are spectroscopic binaries; it is possible that the peculiar profiles may have multiple causes among different objects. The origin and future of these stars are intriguing; for instance, they could be stellar mergers and/or gamma-ray-burst progenitors.
format Articulo
Articulo
author Walborn, Nolan Revere
Howarth, Ian D.
Evans, Christopher J.
Crowther, Paul A.
Moffat, Anthony F. J.
St-Louis, Nicole
Fariña, Cecilia
Bosch, Guillermo Luis
Morrell, Nidia Irene
Barbá, Rodolfo Héctor
Loon, Jacco T. van
author_facet Walborn, Nolan Revere
Howarth, Ian D.
Evans, Christopher J.
Crowther, Paul A.
Moffat, Anthony F. J.
St-Louis, Nicole
Fariña, Cecilia
Bosch, Guillermo Luis
Morrell, Nidia Irene
Barbá, Rodolfo Héctor
Loon, Jacco T. van
author_sort Walborn, Nolan Revere
title The Onfp class in the Magellanic Clouds
title_short The Onfp class in the Magellanic Clouds
title_full The Onfp class in the Magellanic Clouds
title_fullStr The Onfp class in the Magellanic Clouds
title_full_unstemmed The Onfp class in the Magellanic Clouds
title_sort onfp class in the magellanic clouds
publishDate 2010
url http://sedici.unlp.edu.ar/handle/10915/82516
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