A multiwavelength study of the H ii region G347.600 + 00.211 and its effects on the surrounding medium

Autor: Silvina Cichowolski, S B Cárdenas, L. Rizzo, J. A. Molina Lera, L. A. Suad, Roberto Claudio Gamen

Publikováno v: Monthly Notices of the Royal Astronomical Society. 509:3395-3409

We present a multiwavelength investigation of the H ii region G347.600+00.211, located at a distance of 7.9 kpc. We analyse the gas and dust properties aiming to disentangle the origin of the region as well as its role in the formation of new stars.

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::2c8c483794cfe74c42a1a45a487426fd
https://doi.org/10.1093/mnras/stab3084

GS 121–05–037: A new Galactic chimney candidate with signs of triggered star formation

Autor: L. A. Suad, J. A. Molina Lera, S. Cichowolski

Publikováno v: Astronomy & Astrophysics. 668:A44

Aims. The goal of this study is to analyze the H i supershell GS 121–05–037 and its role in triggering star formation. Methods. To characterize the supershell, we analyzed the H i 21-cm line and the far-infrared emission distributions. In additio

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::35d91b2ebde32fc0c9df9e79e40e4c47
https://doi.org/10.1051/0004-6361/202243942

A multi-wavelength analysis of the diffuse HII region G25.8700+0.1350

Autor: Estela Marta Reynoso, N. U. Duronea, L. A. Suad, Silvina Cichowolski, Ricardo Dorda

Publikováno v: CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)

We present a multiwavelength investigation of the HII region G25.8700+0.1350, located in the inner part of the Galaxy. In radio continuum emission, the region is seen as a bright arc-shaped structure. An analysis of the HI line suggests that G25.8700

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9d6a5963c5f00c16a10f07159dd417f6
http://arxiv.org/abs/1710.02835

Triggered star formation in a molecular shell created by a SNR?

Autor: Serge Pineault, Edmundo Marcelo Arnal, L. A. Suad, Silvina Cichowolski, M. E. Ortega, Roberto Claudio Gamen

Publikováno v: CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP

We present a study of a new molecular shell, G 126.1-0.8-14, using available multiwavelength Galactic plane surveys and optical Gemini observations. A well-defined shell-like structure is observed in the CO(1-0) line emission at (l,b) = (126°.1, -0�

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::788db70ba954d0d3bf518c3537de2f42
https://doi.org/10.1093/mnras/stt2259

The infrared and molecular environment surrounding the Wolf-Rayet star WR 130

Autor: Serge Pineault, Silvina Cichowolski, Alberto Noriega-Crespo, N. Flagey, Edmundo Marcelo Arnal, L. A. Suad

Publikováno v: CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP

We present a study of the molecular CO gas and mid/far-infrared radiation arising from the environment surrounding the Wolf-Rayet (WR) star 130. We use the multiwavelength data to analyse the properties of the dense gas and dust, and its possible spa

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d5334cee7dcca795e7c1270aa1df7f72
https://academic.oup.com/mnras/article-abstract/450/4/3458/992360/The-infrared-and-molecular-environment-surrounding?redirectedFrom=fulltext