Ultraviolet extinction toward a quiescent molecular cloud in the Small Magellanic Cloud
Context. The mean UV extinction law for the Small Magellanic Cloud (SMC) is usually taken as a template for low-metallicity galaxies. However, its current derivation is based on only five stars, which renders its universality questionable. More targets with measured extinction laws in the SMC are ne...
| Autores: | , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2012 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/423586 |
| Acceso en línea: | http://hdl.handle.net/10261/423586 |
| Access Level: | acceso abierto |
| Palabra clave: | Dust, extinction Magellanic Clouds Ultraviolet: ISM Tars: early-type |
| Sumario: | Context. The mean UV extinction law for the Small Magellanic Cloud (SMC) is usually taken as a template for low-metallicity galaxies. However, its current derivation is based on only five stars, which renders its universality questionable. More targets with measured extinction laws in the SMC are necessary to determine its possible dependence on parameters such as metallicity and star-forming activity. |
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