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Part of book or chapter of book . 1996 . Peer-reviewed

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Dust and Stars in the Nuclear Region of M51

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Other literature type 01 Jan 1996Publisher:Springer Netherlands

Authors: N. Panagia; S. Scuderi; A. Capetti; Robert P. Kirshner; H. Lamers;

doi: 10.1007/978-94-009-0335-7_78

Dust and Stars in the Nuclear Region of M51

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Abstract

The observations were made with the Hubble Space Telescope (HST) 1 as part of the SINS (Supernova INtensive Study) project, to determine accurate UV (early epoch) and optical (late epoch) magnitudes of SNIc 1994I, which occurred about 15″ offset from M51 nucleus. In particular, we have HST-WFPC2 images obtained on 1994 May 12, with the F255W and F336W filters (in these images the nucleus falls in WF2), and four more taken on 1995 January 15 with the F439W, F555W, F675W, and F814W filters (the nucleus is in PC1).

Related Organizations

Harvard University
United States
University Museum Utrecht
Netherlands

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