The ISM around WR 152 and WR 153ab
We analyzed the distribution of the interstellar matter in the environs of the WR stars WR152 and WR153ab, associated with ring nebulae in the Sh2-132 Hii region. Our study is based on radio data (continuum, Hi, and CO(1-0) observations) and images in the far and mid IR. We have detected the radio c...
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Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_14052059_v33_n_p142_Cappa |
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todo:paper_14052059_v33_n_p142_Cappa2023-10-03T16:12:57Z The ISM around WR 152 and WR 153ab Cappa, C.E. Vasquez, J. Arnal, E.M. Cichowolski, S. Pineault, S. ISM: ring nebulae Stars: individual (WR152, WR153AB) Stars: wolf-rayet We analyzed the distribution of the interstellar matter in the environs of the WR stars WR152 and WR153ab, associated with ring nebulae in the Sh2-132 Hii region. Our study is based on radio data (continuum, Hi, and CO(1-0) observations) and images in the far and mid IR. We have detected the radio continuum and far IR counterparts of the ionized shells related to WR152, as well as Hi gas linked to the outer ionized shell. The distributions of the ionized and molecular gas related to WR153ab and that of the PAHs suggest the presence of photodissociation regions at the interface between the ionized and molecular material. We estimate the main physical parameters of the gas components. © 2008: Instituto de Astronomía. CONF info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_14052059_v33_n_p142_Cappa |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
ISM: ring nebulae Stars: individual (WR152, WR153AB) Stars: wolf-rayet |
spellingShingle |
ISM: ring nebulae Stars: individual (WR152, WR153AB) Stars: wolf-rayet Cappa, C.E. Vasquez, J. Arnal, E.M. Cichowolski, S. Pineault, S. The ISM around WR 152 and WR 153ab |
topic_facet |
ISM: ring nebulae Stars: individual (WR152, WR153AB) Stars: wolf-rayet |
description |
We analyzed the distribution of the interstellar matter in the environs of the WR stars WR152 and WR153ab, associated with ring nebulae in the Sh2-132 Hii region. Our study is based on radio data (continuum, Hi, and CO(1-0) observations) and images in the far and mid IR. We have detected the radio continuum and far IR counterparts of the ionized shells related to WR152, as well as Hi gas linked to the outer ionized shell. The distributions of the ionized and molecular gas related to WR153ab and that of the PAHs suggest the presence of photodissociation regions at the interface between the ionized and molecular material. We estimate the main physical parameters of the gas components. © 2008: Instituto de Astronomía. |
format |
CONF |
author |
Cappa, C.E. Vasquez, J. Arnal, E.M. Cichowolski, S. Pineault, S. |
author_facet |
Cappa, C.E. Vasquez, J. Arnal, E.M. Cichowolski, S. Pineault, S. |
author_sort |
Cappa, C.E. |
title |
The ISM around WR 152 and WR 153ab |
title_short |
The ISM around WR 152 and WR 153ab |
title_full |
The ISM around WR 152 and WR 153ab |
title_fullStr |
The ISM around WR 152 and WR 153ab |
title_full_unstemmed |
The ISM around WR 152 and WR 153ab |
title_sort |
ism around wr 152 and wr 153ab |
url |
http://hdl.handle.net/20.500.12110/paper_14052059_v33_n_p142_Cappa |
work_keys_str_mv |
AT cappace theismaroundwr152andwr153ab AT vasquezj theismaroundwr152andwr153ab AT arnalem theismaroundwr152andwr153ab AT cichowolskis theismaroundwr152andwr153ab AT pineaults theismaroundwr152andwr153ab AT cappace ismaroundwr152andwr153ab AT vasquezj ismaroundwr152andwr153ab AT arnalem ismaroundwr152andwr153ab AT cichowolskis ismaroundwr152andwr153ab AT pineaults ismaroundwr152andwr153ab |
_version_ |
1807317357185466368 |