SN 2005kd: another very luminous, slowly declining type IIn supernova

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dc.creatorTsvetkov, D. Yu.
dc.date2008-03-27
dc.date.accessioned2026-07-07T10:12:16Z
dc.date.available2026-07-07T10:12:16Z
dc.descriptionCCD UBVRI photometry is presented for type IIn SN 2005kd. The maximum luminosity exceeded Mv=-19.8, and SN remained brighter than -18 mag for about 400 days. While overall photometric evolution is quite similar to SN 1997cy, SN 2005kd shows a plateau at phases between 119 and 311 days past explosion, which is a unique feature for SN IIn.
dc.description8 pages, 5 figures, submitted to Variable Stars
dc.identifierhttps://arxiv.org/abs/0803.3906
dc.identifierhttp://arxiv.org/abs/0803.3906
dc.identifierPeremennye Zvezdy (Variable Stars), 2008, vol. 28, N 6
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/172126
dc.subjectAstrophysics
dc.titleSN 2005kd: another very luminous, slowly declining type IIn supernova
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