Registro completo de metadatos
| Campo DC | Valor | Lengua/Idioma |
|---|---|---|
| dc.creator | Benaglia, Paula | - |
| dc.creator | Dougherty, S. M. | - |
| dc.creator | Phillips, C. | - |
| dc.creator | Koribalski, B. | - |
| dc.creator | Tzioumis, T. | - |
| dc.date | 2016-07-04T16:37:39Z | - |
| dc.date | 2016-07-04T16:37:39Z | - |
| dc.date | 2010-02 | - |
| dc.date | 2016-06-15T19:20:11Z | - |
| dc.date.accessioned | 2019-04-29T15:52:11Z | - |
| dc.date.available | 2019-04-29T15:52:11Z | - |
| dc.date.issued | 2010-02 | - |
| dc.identifier | Benaglia, Paula; Dougherty, S. M.; Phillips, C.; Koribalski, B.; Tzioumis, T.; HD 93129A at different radio scales; Universidad Nacional Autónoma de México. Instituto de Astronomía; Revista Mexicana de Astronomía y Astrofísica; 38; 2-2010; 41-42 | - |
| dc.identifier | 0185-1101 | - |
| dc.identifier | http://hdl.handle.net/11336/6325 | - |
| dc.identifier.uri | http://rodna.bn.gov.ar:8080/jspui/handle/bnmm/304172 | - |
| dc.description | Recent observations toward the O2 If* star HD 93129A have revealed important non-thermal radio emission, and that it has an early O companion 140 AU away if at 2.5 kpc (FGS-HST data). These facts strongly support the possibility of a massive stars wind-collision region as the acceleration site of the synchrotron-emitting relativistic electrons. We have carried out LBA VLBI observations at 2.37 GHz to resolve the non-thermal source, and search for a bow-shock shape, typical of a wind-collision region. Preliminary results are presented here. | - |
| dc.description | Fil: Benaglia, Paula. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto Argentino de Radioastronomia (i); Argentina | - |
| dc.description | Fil: Dougherty, S. M.. National Research Council of Canada, Herzberg Institute for Astrophysics, Dominion Radio Astrophysical Observatory; Canadá | - |
| dc.description | Fil: Phillips, C.. Australia Telescope National Facility, CSIRO; Australia | - |
| dc.description | Fil: Koribalski, B.. Australia Telescope National Facility, CSIRO; Australia | - |
| dc.description | Fil: Tzioumis, T.. Australia Telescope National Facility, CSIRO; Australia | - |
| dc.format | application/pdf | - |
| dc.format | application/pdf | - |
| dc.language | eng | - |
| dc.publisher | Universidad Nacional Autónoma de México. Instituto de Astronomía | - |
| dc.relation | info:eu-repo/semantics/altIdentifier/url/http://www.astroscu.unam.mx/rmaa/RMxAC..38/PDF/RMxAC..38_pbenaglia.pdf | - |
| dc.relation | info:eu-repo/semantics/altIdentifier/url/http://www.redalyc.org/articulo.oa?id=57115706015 | - |
| dc.rights | info:eu-repo/semantics/openAccess | - |
| dc.rights | https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ | - |
| dc.source | reponame:CONICET Digital (CONICET) | - |
| dc.source | instname:Consejo Nacional de Investigaciones Científicas y Técnicas | - |
| dc.source | instacron:CONICET | - |
| dc.subject | Radiation mechanisms | - |
| dc.subject | HD93129A (estrella) | - |
| dc.subject | Winds | - |
| dc.subject | Nonthermal mechanisms | - |
| dc.subject | Stellar winds | - |
| dc.subject | Outflows. | - |
| dc.subject | Astronomía | - |
| dc.subject | Ciencias Físicas | - |
| dc.subject | CIENCIAS NATURALES Y EXACTAS | - |
| dc.title | HD 93129A at different radio scales | - |
| dc.type | info:eu-repo/semantics/article | - |
| dc.type | info:eu-repo/semantics/publishedVersion | - |
| dc.type | info:ar-repo/semantics/articulo | - |
| Aparece en las colecciones: | CONICET | |
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