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Spectroscopic and Photometric Observations of SN IIn 1995N

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arxiv astro-ph/0504116 v1 pith:MHPQ4TO5 submitted 2005-04-05 astro-ph

A. Pastorello , I. Aretxaga , L. Zampieri , P. Mucciarelli , S. Benetti This is my paper · ORCID
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We present the results of a long-term program of monitoring of the famous SN 1995N, observed both in photometry (UBVRIJHK bands) and optical spectroscopy. The observations span a period of about 9 years. These new data, together with others available in literature, extend from the X-ray wavelengths to the radio, and allow to estimate the total energy radiated by the supernova over a decade after its explosion.

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  1. Very Late-Time JWST and Keck Spectra of the Oxygen-Rich Supernova 1995N

    astro-ph.SR 2025-05 conditional novelty 6.0 of 10

    SN 1995N, observed 28 years after explosion, shows oxygen lines stronger than H-alpha, marking the start of its transition from supernova to supernova remnant, while its infrared dust emission continues at reduced luminosity.

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