Pre main sequence stars as UV sources for the World Space Observatory-UV mission
| dc.contributor.author | Gómez De Castro, Ana Inés | |
| dc.contributor.author | Lamzin, Sergei A. | |
| dc.date.accessioned | 2023-06-20T00:13:38Z | |
| dc.date.available | 2023-06-20T00:13:38Z | |
| dc.date.issued | 2011-09 | |
| dc.description.abstract | Pre-main sequence stars are bright UV (UV) sources compared with their main sequence analogues. The source of this excess is the high energy processes associated with the physics of accretion/outflow during early stellar evolution. In this review, the main sources of UV excess are described as well as the most significant "unknowns" in the field. Special emphasis is made on the results from the last observations carried out with the Hubble Space Telescope and on the relevance of future dedicated monitoring programs with the World Space Observatory-UV. | en |
| dc.description.department | Unidad Deptal. de Astronomía y Geodesia | |
| dc.description.faculty | Fac. de Ciencias Matemáticas | |
| dc.description.refereed | TRUE | |
| dc.description.sponsorship | Ministerio de Ciencia, Innovación y Universidades (España) | |
| dc.description.status | pub | |
| dc.eprint.id | https://eprints.ucm.es/id/eprint/15860 | |
| dc.identifier.citation | Gómez de Castro, A. I. & Lamzin, S. A. «Pre Main Sequence Stars as UV Sources for the World Space Observatory-UV Mission». Astrophysics and Space Science, vol. 335, n.o 1, septiembre de 2011, pp. 61-68. DOI.org (Crossref), https://doi.org/10.1007/s10509-011-0649-2. | |
| dc.identifier.doi | 10.1007/s10509-011-0649-2 | |
| dc.identifier.issn | 0004-640X | |
| dc.identifier.officialurl | https//doi.org/10.1007/s10509-011-0649-2 | |
| dc.identifier.relatedurl | http://www.springerlink.com/content/mk71847u6n384761/fulltext.pdf | |
| dc.identifier.uri | https://hdl.handle.net/20.500.14352/42230 | |
| dc.issue.number | 1 | |
| dc.journal.title | Astrophysics and space science | |
| dc.language.iso | eng | |
| dc.page.final | 68 | |
| dc.page.initial | 61 | |
| dc.publisher | Springer | |
| dc.relation.projectID | AYA2008-06423 | |
| dc.rights.accessRights | restricted access | |
| dc.subject.cdu | 52 | |
| dc.subject.keyword | T-tauri stars | |
| dc.subject.keyword | Herbig ae/be stars | |
| dc.subject.keyword | Young stars | |
| dc.subject.keyword | Ab-aurigae | |
| dc.subject.keyword | Mg-ii | |
| dc.subject.keyword | Dense outflows | |
| dc.subject.keyword | Bp tauri | |
| dc.subject.keyword | Ultraviolet | |
| dc.subject.keyword | Accretion | |
| dc.subject.keyword | Line | |
| dc.subject.ucm | Astronomía (Matemáticas) | |
| dc.subject.unesco | 21 Astronomía y Astrofísica | |
| dc.title | Pre main sequence stars as UV sources for the World Space Observatory-UV mission | en |
| dc.type | journal article | |
| dc.volume.number | 335 | |
| dspace.entity.type | Publication | |
| relation.isAuthorOfPublication | 492947a5-78aa-4c19-bb69-3dd332bff97c | |
| relation.isAuthorOfPublication.latestForDiscovery | 492947a5-78aa-4c19-bb69-3dd332bff97c |
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