A Long-duration Luminous Type IIn Supernova KISS15s: Strong Recombination Lines from the Inhomogeneous Ejecta–CSM Interaction Region and Hot Dust Emission from Newly Formed Dust-Reference-Cited by-同舟云学术

A Long-duration Luminous Type IIn Supernova KISS15s: Strong Recombination Lines from the Inhomogeneous Ejecta–CSM Interaction Region and Hot Dust Emission from Newly Formed Dust

Published:2019-02-19 Issue:2 Volume:872 Page:135
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Kokubo Mitsuru^ORCID,Mitsuda Kazuma^ORCID,Morokuma Tomoki,Tominaga Nozomu^ORCID,Tanaka Masaomi^ORCID,Moriya Takashi J.^ORCID,Yoachim Peter^ORCID,Ivezić Željko,Sako Shigeyuki,Doi Mamoru

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/872/i=2/a=135/pdf

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1. THE DETECTION OF A SN IIn IN OPTICAL FOLLOW-UP OBSERVATIONS OF ICECUBE NEUTRINO EVENTS

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3. Early dust formation and a massive progenitor for SN 2011ja?

4. THE SLOAN DIGITAL SKY SURVEY COADD: 275 deg2OF DEEP SLOAN DIGITAL SKY SURVEY IMAGING ON STRIPE 82

5. SN 1988Z: spectro-photometric catalogue and energy estimates

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