Multiwavelength study of RCW 108 as a massive star forming region

NGC 6193 is an open cluster embedded in an Hii region (RCW 108, Rodgers et al. 1960) located 15 0 eastwards of NGC 6188. The later is a bright rimmed cloud that stretches over 30 0 in the north-south direction, and marks the interface between RCW 108 and nearby dark clouds. RCW 108 is being powered...

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Detalles Bibliográficos
Autores principales: Romero, Gisela Andrea, Barbá, Rodolfo Héctor, Arnal, Edmundo Marcelo
Formato: Articulo
Lenguaje:Inglés
Publicado: 2008
Materias:
Ciencias Astronómicas
Stellar formation
NGC 6193 (galaxia)
Hii regions
Interstellar medium
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/99614
https://ri.conicet.gov.ar/11336/22325
http://adsabs.harvard.edu/abs/2008RMxAC..33..166R
http://www.astroscu.unam.mx/rmaa/RMxAC..33/PDF/RMxAC..33_garomero.pdf
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata
id I19-R120-10915-99614
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
Stellar formation
NGC 6193 (galaxia)
Hii regions
Interstellar medium
spellingShingle Ciencias Astronómicas
Stellar formation
NGC 6193 (galaxia)
Hii regions
Interstellar medium
Romero, Gisela Andrea
Barbá, Rodolfo Héctor
Arnal, Edmundo Marcelo
Multiwavelength study of RCW 108 as a massive star forming region
topic_facet Ciencias Astronómicas
Stellar formation
NGC 6193 (galaxia)
Hii regions
Interstellar medium
description NGC 6193 is an open cluster embedded in an Hii region (RCW 108, Rodgers et al. 1960) located 15 0 eastwards of NGC 6188. The later is a bright rimmed cloud that stretches over 30 0 in the north-south direction, and marks the interface between RCW 108 and nearby dark clouds. RCW 108 is being powered by the multiple O-type star systems, namely HD 150135-HD 150136 (Niemela & Gamen 2005) in the core of NGC 6193. The UV photons emitted by these stars may drive photoinization-induced shocks into the nearby molecular clouds, possibly originating the well studied infrared cluster RCW108- IR (Comerón et al. 2005, and references therein). In this work we describe the morphology of the distribution of the photoionized and shock-excited gas based on Hα, [O III] and [S II] images, 13CO observations, and infrared data (2MASS, MSX).
format Articulo
Articulo
author Romero, Gisela Andrea
Barbá, Rodolfo Héctor
Arnal, Edmundo Marcelo
author_facet Romero, Gisela Andrea
Barbá, Rodolfo Héctor
Arnal, Edmundo Marcelo
author_sort Romero, Gisela Andrea
title Multiwavelength study of RCW 108 as a massive star forming region
title_short Multiwavelength study of RCW 108 as a massive star forming region
title_full Multiwavelength study of RCW 108 as a massive star forming region
title_fullStr Multiwavelength study of RCW 108 as a massive star forming region
title_full_unstemmed Multiwavelength study of RCW 108 as a massive star forming region
title_sort multiwavelength study of rcw 108 as a massive star forming region
publishDate 2008
url http://sedici.unlp.edu.ar/handle/10915/99614
https://ri.conicet.gov.ar/11336/22325
http://adsabs.harvard.edu/abs/2008RMxAC..33..166R
http://www.astroscu.unam.mx/rmaa/RMxAC..33/PDF/RMxAC..33_garomero.pdf
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AT barbarodolfohector multiwavelengthstudyofrcw108asamassivestarformingregion
AT arnaledmundomarcelo multiwavelengthstudyofrcw108asamassivestarformingregion
bdutipo_str Repositorios
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