E-BOSS: An Extensive stellar BOw Shock Survey : II. Catalogue second release

Context. Stellar bow shocks have been studied not only observationally, but also theoretically since the late 1980s. Only a few catalogues of them exist. The bow shocks show emission along all the electromagnetic spectrum, but they are detected more easily in infrared wavelengths. The release of new...

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Autores principales: Peri, Cintia Soledad, Benaglia, Paula, Isequilla, Natacha Laura
Formato: Articulo
Lenguaje:Inglés
Publicado: 2015
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/86397
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id I19-R120-10915-86397
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
Catalogs
Infrared: ISM
Stars: early-type
spellingShingle Ciencias Astronómicas
Catalogs
Infrared: ISM
Stars: early-type
Peri, Cintia Soledad
Benaglia, Paula
Isequilla, Natacha Laura
E-BOSS: An Extensive stellar BOw Shock Survey : II. Catalogue second release
topic_facet Ciencias Astronómicas
Catalogs
Infrared: ISM
Stars: early-type
description Context. Stellar bow shocks have been studied not only observationally, but also theoretically since the late 1980s. Only a few catalogues of them exist. The bow shocks show emission along all the electromagnetic spectrum, but they are detected more easily in infrared wavelengths. The release of new and high-quality infrared data eases the discovery and subsequent study of new objects. Aims. We search stellar bow-shock candidates associated with nearby runaway stars, and gather them together with those found elsewhere, to enlarge the list of the E-BOSS first release. We aim to characterize the bow-shock candidates and provide a database suitable for statistical studies. We investigate the low-frequency radio emission at the position of the bow-shock features, that can contribute to further studies of high-energy emission from these objects. Methods. We considered samples from different literature sources and searched for bow-shaped structures associated with stars in the Wide-field Infrared Survey Explorer (WISE) images. We looked for each bow-shock candidate on centimeter radio surveys. Results. We reunited 45 bow-shock candidates and generated composed WISE images to show the emission in different infrared bands. Among them there are new sources, previously studied objects, and bow shocks found serendipitously. Five bow shocks show evidence of radio emission. Conclusions. Stellar bow shocks constitute an active field with open questions and enormous amounts of data to be analyzed. Future research at all wavelengths databases, and use of instruments like Gaia, will provide a more complete picture of these objects. For instance, infrared spectral energy distributions can give information about physical parameters of the bow shock matter. In addition, dedicated high-sensitivity radio observations can help to understand the radio-γ connection.
format Articulo
Articulo
author Peri, Cintia Soledad
Benaglia, Paula
Isequilla, Natacha Laura
author_facet Peri, Cintia Soledad
Benaglia, Paula
Isequilla, Natacha Laura
author_sort Peri, Cintia Soledad
title E-BOSS: An Extensive stellar BOw Shock Survey : II. Catalogue second release
title_short E-BOSS: An Extensive stellar BOw Shock Survey : II. Catalogue second release
title_full E-BOSS: An Extensive stellar BOw Shock Survey : II. Catalogue second release
title_fullStr E-BOSS: An Extensive stellar BOw Shock Survey : II. Catalogue second release
title_full_unstemmed E-BOSS: An Extensive stellar BOw Shock Survey : II. Catalogue second release
title_sort e-boss: an extensive stellar bow shock survey : ii. catalogue second release
publishDate 2015
url http://sedici.unlp.edu.ar/handle/10915/86397
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