Registro completo de metadatos
| Campo DC | Valor | Lengua/Idioma |
|---|---|---|
| dc.creator | Rivera Sandoval, L. E. | - |
| dc.creator | van den Berg, M. | - |
| dc.creator | Heinke, C. O. | - |
| dc.creator | Cohn, H. N | - |
| dc.creator | Lugger, P. M | - |
| dc.creator | Freire, P. | - |
| dc.creator | Anderson, J. | - |
| dc.creator | Serenelli, A. M. | - |
| dc.creator | Althaus, Leandro Gabriel | - |
| dc.creator | Cool, A. M. | - |
| dc.creator | Grindlay, J. E | - |
| dc.creator | Edmonds, P. D. | - |
| dc.creator | Wijnands, R. | - |
| dc.creator | Ivanova, N. | - |
| dc.date | 2017-01-05T17:18:00Z | - |
| dc.date | 2017-01-05T17:18:00Z | - |
| dc.date | 2015-11 | - |
| dc.date | 2017-01-02T18:36:57Z | - |
| dc.date.accessioned | 2019-04-29T15:41:03Z | - |
| dc.date.available | 2019-04-29T15:41:03Z | - |
| dc.date.issued | 2017-01-05T17:18:00Z | - |
| dc.date.issued | 2017-01-05T17:18:00Z | - |
| dc.date.issued | 2015-11 | - |
| dc.date.issued | 2017-01-02T18:36:57Z | - |
| dc.identifier | Rivera Sandoval, L. E.; van den Berg, M.; Heinke, C. O.; Cohn, H. N; Lugger, P. M; et al.; Discovery of near-ultraviolet counterparts to millisecond pulsars in the globular cluster 47 Tucanae; Wiley Blackwell Publishing, Inc; Monthly Notices Of The Royal Astronomical Society; 453; 3; 11-2015; 2707-2717 | - |
| dc.identifier | 0035-8711 | - |
| dc.identifier | http://hdl.handle.net/11336/10870 | - |
| dc.identifier.uri | http://rodna.bn.gov.ar:8080/jspui/handle/bnmm/299447 | - |
| dc.description | We report the discovery of the likely white dwarf companions to radiomillisecond pulsars 47 Tuc Q and 47 Tuc S in the globular cluster 47Tucanae. These blue stars were found in near-ultraviolet images from theHubble Space Telescope for which we derived accurate absoluteastrometry, and are located at positions consistent with the radiocoordinates to within 0.016 arcsec (0.2σ). We presentnear-ultraviolet and optical colours for the previously identifiedcompanion to millisecond pulsar 47 Tuc U, and we unambiguously confirmthe tentative prior identifications of the optical counterparts to 47Tuc T and 47 Tuc Y. For the latter, we present its radio-timing solutionfor the first time. We find that all five near-ultraviolet counterpartshave U<sub>300</sub> - B<sub>390</sub> colours that are consistent withHe white dwarf cooling models for masses ?0.16-0.3M<sub>⊙</sub> and cooling ages within ?0.1-6 Gyr. The Hα- R<sub>625</sub> colours of 47 Tuc U and 47 Tuc T indicate the presenceof a strong Hα absorption line, as expected for white dwarfs withan H envelope.<hr /> | - |
| dc.description | Fil: Rivera Sandoval, L. E.. University Of Amsterdam; Países Bajos | - |
| dc.description | Fil: van den Berg, M.. University Of Amsterdam; Países Bajos. Harvard–Smithsonian Center for Astrophysics; Estados Unidos | - |
| dc.description | Fil: Heinke, C. O.. University of Alberta; Canadá. Max Planck Institute for Radio Astronomy; Alemania | - |
| dc.description | Fil: Cohn, H. N. Indiana University; Estados Unidos | - |
| dc.description | Fil: Lugger, P. M. Indiana University; Estados Unidos | - |
| dc.description | Fil: Freire, P.. Max Planck Institute for Radio Astronomy; Alemania | - |
| dc.description | Fil: Anderson, J.. Space Telescope Science Institute; Estados Unidos | - |
| dc.description | Fil: Serenelli, A. M.. Instituto de Ciencias del Espacio (CSIC-IEEC); España | - |
| dc.description | Fil: Althaus, Leandro Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina | - |
| dc.description | Fil: Cool, A. M.. San Francisco State University; Estados Unidos | - |
| dc.description | Fil: Grindlay, J. E. Harvard-Smithsonian Center for Astrophysics; Estados Unidos | - |
| dc.description | Fil: Edmonds, P. D.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos | - |
| dc.description | Fil: Wijnands, R.. University Of Amsterdam; Países Bajos | - |
| dc.description | Fil: Ivanova, N.. University of Alberta; Canadá | - |
| dc.format | application/pdf | - |
| dc.format | application/pdf | - |
| dc.language | eng | - |
| dc.publisher | Wiley Blackwell Publishing, Inc | - |
| dc.relation | info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1093/mnras/stv1810 | - |
| dc.relation | info:eu-repo/semantics/altIdentifier/url/http://mnras.oxfordjournals.org/content/453/3/2707 | - |
| 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 | white dwarfs | - |
| dc.subject | stellar populations | - |
| dc.subject | Astronomía | - |
| dc.subject | Ciencias Físicas | - |
| dc.subject | CIENCIAS NATURALES Y EXACTAS | - |
| dc.title | Discovery of near-ultraviolet counterparts to millisecond pulsars in the globular cluster 47 Tucanae | - |
| 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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