Photometry of Nova V 1493 Aql

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dc.creatorBonifacio, Piercarlo
dc.creatorSelvelli, Pierluigi
dc.creatorCaffau, Elisabetta
dc.date2000-03-11
dc.date.accessioned2026-07-07T01:52:42Z
dc.date.available2026-07-07T01:52:42Z
dc.descriptionWe report on photometric observations of V 1493 Aql during the early decline and highlight some uncommon aspects of the light curve. V 1493 Aql was hotter at maximum light than in the following phases, and was characterized by the presence of a long lasting secondary maximum, that, unlike in other novae, was quite red in color. The mean of three distance estimates yields d ~ 18.8 +/- 3.6 Kpc. Such a large distance would place V 1493 Aql at the extreme outskirts of our Galaxy or even in an external Local Group galaxy.
dc.descriptionTo be published in A&A Letters
dc.identifierhttps://arxiv.org/abs/astro-ph/0003156
dc.identifierhttp://arxiv.org/abs/astro-ph/0003156
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/707
dc.subjectAstrophysics
dc.titlePhotometry of Nova V 1493 Aql
dc.typetext

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