Photometric and spectroscopic study of a highly reddened type Ia
supernova SN 2003hx in NGC 2076

dc.contributor.author	Misra, K.
dc.contributor.author	Sahu, D. K.
dc.contributor.author	Anupama, G. C.
dc.contributor.author	Pandey, K.
dc.date.accessioned	2009-06-19T10:27:36Z
dc.date.available	2009-06-19T10:27:36Z
dc.date.issued	2008
dc.identifier.uri	http://hdl.handle.net/123456789/47
dc.description.abstract	We present UBVRI CCD photometry and optical spectra of the type Ia supernova SN 2003hx which appeared in the galaxy NGC 2076, obtained till ∼ 146 d after the epoch of B-band maximum. The supernova reached at maximum brightness in B band on JD 245 2893 ± 1.0 with an apparent magnitude of 14.92 ± 0.01 mag which was estimated by making template fits to the light curves. SN 2003hx is an example of a highly reddened supernova with E(B − V) = 0.56 ± 0.23. The spectral evolution indicates the supernova to be a normal type Ia event.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	mn389-706
dc.subject	Supernovae, General – supernovae, Individual, SN 2003hx – galaxies, Individual, NGC 2076	en_US
dc.title	Photometric and spectroscopic study of a highly reddened type Ia supernova SN 2003hx in NGC 2076	en_US
dc.type	Article	en_US