A dust bubble within the globular cluster NGC 6624?

A multi-color analysis of CCD frames and polarimetry for both dark patches and stars in the field of the globular cluster NGC 6624 is presented. Several of these patches have a wavelength behavior that is consistent with the existence of intra-cluster dust. The spatial distribution of these patches...

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Autores principales: Forte, Juan Carlos, Cellone, Sergio Aldo, Méndez, Mariano R., Vega, Ema Irene
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1990
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/143163
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id I19-R120-10915-143163
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spelling I19-R120-10915-1431632024-04-18T18:50:21Z http://sedici.unlp.edu.ar/handle/10915/143163 A dust bubble within the globular cluster NGC 6624? Forte, Juan Carlos Cellone, Sergio Aldo Méndez, Mariano R. Vega, Ema Irene 1990 2022-10-03T12:04:30Z es Astronomía Galaxia A multi-color analysis of CCD frames and polarimetry for both dark patches and stars in the field of the globular cluster NGC 6624 is presented. Several of these patches have a wavelength behavior that is consistent with the existence of intra-cluster dust. The spatial distribution of these patches is not at random, rather, they appear distributed on a circular pattern some 2 parsecs in radius. Remarkably, the center of this structure, that seems to be a "bubble", is not far from the position of the X ray burster 1820-30. A possible connection between these objects might suggest the existence of an explosive event in the past. Asociación Argentina de Astronomía Articulo Comunicacion http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Español
topic Astronomía
Galaxia
spellingShingle Astronomía
Galaxia
Forte, Juan Carlos
Cellone, Sergio Aldo
Méndez, Mariano R.
Vega, Ema Irene
A dust bubble within the globular cluster NGC 6624?
topic_facet Astronomía
Galaxia
description A multi-color analysis of CCD frames and polarimetry for both dark patches and stars in the field of the globular cluster NGC 6624 is presented. Several of these patches have a wavelength behavior that is consistent with the existence of intra-cluster dust. The spatial distribution of these patches is not at random, rather, they appear distributed on a circular pattern some 2 parsecs in radius. Remarkably, the center of this structure, that seems to be a "bubble", is not far from the position of the X ray burster 1820-30. A possible connection between these objects might suggest the existence of an explosive event in the past.
format Articulo
Comunicacion
author Forte, Juan Carlos
Cellone, Sergio Aldo
Méndez, Mariano R.
Vega, Ema Irene
author_facet Forte, Juan Carlos
Cellone, Sergio Aldo
Méndez, Mariano R.
Vega, Ema Irene
author_sort Forte, Juan Carlos
title A dust bubble within the globular cluster NGC 6624?
title_short A dust bubble within the globular cluster NGC 6624?
title_full A dust bubble within the globular cluster NGC 6624?
title_fullStr A dust bubble within the globular cluster NGC 6624?
title_full_unstemmed A dust bubble within the globular cluster NGC 6624?
title_sort dust bubble within the globular cluster ngc 6624?
publishDate 1990
url http://sedici.unlp.edu.ar/handle/10915/143163
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AT fortejuancarlos dustbubblewithintheglobularclusterngc6624
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