A new catalog of HI supershell candidates in the outer part of the Galaxy

Aims. The main goal of this work is to a have a new neutral hydrogen (H i) supershell candidate catalog to analyze their spatial distribution in the Galaxy and to carry out a statistical study of their main properties. Methods. This catalog was carried out making use of the Leiden-Argentine-Bonn (L...

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Detalles Bibliográficos
Autores principales: Suad, Laura Andrea, Caiafa, Cesar F., Arnal, Edmundo Marcelo, Cichowolski, Silvina
Formato: Articulo Preprint
Lenguaje:Inglés
Publicado: 2014
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/123541
Aporte de:
id I19-R120-10915-123541
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
ISM: bubbles
ISM: structure
Methods: data analysis
Techniques: image processing
Radio lines: ISM
spellingShingle Ciencias Astronómicas
ISM: bubbles
ISM: structure
Methods: data analysis
Techniques: image processing
Radio lines: ISM
Suad, Laura Andrea
Caiafa, Cesar F.
Arnal, Edmundo Marcelo
Cichowolski, Silvina
A new catalog of HI supershell candidates in the outer part of the Galaxy
topic_facet Ciencias Astronómicas
ISM: bubbles
ISM: structure
Methods: data analysis
Techniques: image processing
Radio lines: ISM
description Aims. The main goal of this work is to a have a new neutral hydrogen (H i) supershell candidate catalog to analyze their spatial distribution in the Galaxy and to carry out a statistical study of their main properties. Methods. This catalog was carried out making use of the Leiden-Argentine-Bonn (LAB) survey. The supershell candidates were identified using a combination of two techniques: a visual inspection plus an automatic searching algorithm. Our automatic algorithm is able to detect both closed and open structures. Results. A total of 566 supershell candidates were identified. Most of them (347) are located in the second Galactic quadrant, while 219 were found in the third one. About 98% of a subset of 190 structures (used to derive the statistical properties of the supershell candidates) are elliptical with a mean weighted eccentricity of 0.8 ± 0.1, and ∼70% have their major axes parallel to the Galactic plane. The weighted mean value of the effective radius of the structures is ∼160 pc. Owing to the ability of our automatic algorithm to detect open structures, we have also identified some “galactic chimney” candidates. We find an asymmetry between the second and third Galactic quadrants in the sense that in the second one we detect structures as far as 32 kpc, while for the 3rd one the farthest structure is detected at 17 kpc. The supershell surface density in the solar neighborhood is ∼8 kpc−2, and decreases as we move farther away form the Galactic center. We have also compared our catalog with those by other authors
format Articulo
Preprint
author Suad, Laura Andrea
Caiafa, Cesar F.
Arnal, Edmundo Marcelo
Cichowolski, Silvina
author_facet Suad, Laura Andrea
Caiafa, Cesar F.
Arnal, Edmundo Marcelo
Cichowolski, Silvina
author_sort Suad, Laura Andrea
title A new catalog of HI supershell candidates in the outer part of the Galaxy
title_short A new catalog of HI supershell candidates in the outer part of the Galaxy
title_full A new catalog of HI supershell candidates in the outer part of the Galaxy
title_fullStr A new catalog of HI supershell candidates in the outer part of the Galaxy
title_full_unstemmed A new catalog of HI supershell candidates in the outer part of the Galaxy
title_sort new catalog of hi supershell candidates in the outer part of the galaxy
publishDate 2014
url http://sedici.unlp.edu.ar/handle/10915/123541
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