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dc.date.accessioned | 2010-08-26T15:00:50Z | |
dc.date.available | 2010-08-26T03:00:00Z | |
dc.date.issued | 2001 | |
dc.identifier.uri | http://sedici.unlp.edu.ar/handle/10915/2063 | |
dc.description.abstract | G. L. Bosch, R. H. Barba, and N. I. Morrell, Observatorio Astronomico, Universidad Nacional de La Plata, report that echelle spectroscopy (range 460-780 nm, resolution 0.04 nm) obtained of the nova at CASLEO Observatory on Oct. 26.149 UT shows strong, low-excitation emission lines of H, Fe II, [O I], O I, Na I, and possibly [Ni I] with broad P-Cyg profiles. Terminal wind velocities measured from the absorption-profile edge in H-beta indicates expansion of up to 1800 km/s, while Fe II and Na I lines show a slower expansion velocity of 950 km/s. The FWHM of the H-alpha emission was about 1400 km/s. | es |
dc.language | en | es |
dc.subject | astrofísica | es |
dc.subject | Estrellas Celestiales | es |
dc.title | Nova in the Small Magellanic Cloud 2001 | en |
dc.type | Articulo | es |
sedici.identifier.uri | http://www.cbat.eps.harvard.edu/iauc/07700/07744.html | es |
sedici.creator.person | Bosch, Guillermo Luis | es |
sedici.creator.person | Barbá, Rodolfo Héctor | es |
sedici.creator.person | Morrell, Nidia Irene | es |
sedici.description.note | Información extraída del sitio web de la Facultad de Ciencias Astronómicas y Geofísicas. | es |
sedici.subject.materias | Ciencias Astronómicas | es |
sedici.description.fulltext | true | es |
mods.originInfo.place | Facultad de Ciencias Astronómicas y Geofísicas | es |
sedici.subtype | Articulo | es |
sedici.rights.license | Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0) | |
sedici.rights.uri | http://creativecommons.org/licenses/by-nc-nd/4.0/ | |
sedici.description.peerReview | peer-review | es |
sedici2003.identifier | ARG-UNLP-ART-0000006362 | es |
sedici.relation.journalTitle | International Astronomical Union Circular | es |
sedici.relation.journalVolumeAndIssue | no. 7744 | es |