Distance of the hypernova SN 2002ap via the expanding photosphere method

Astronomy and Astrophysics

Volumn 427, Issue 2, 2004, Pages 453-464

  Vinko J ^a,e   Blake, R M ^b   Sarneczky K ^a,e   Csak B ^a,e   Furesz G ^c,e   Csizmadia, Sz ^c   Kiss, L L ^a,d   Szabo Gy M ^a,e   Szabo R ^c   DeBond, H ^b   De Robertis, M M ^b   Thomson, J R ^b   Mochnacki, S W ^b  

^a UNIVERSITY OF SZEGED   (Hungary)

^b UNIVERSITY OF TORONTO   (Canada)

^c INSTITUTE OF EXPERIMENTAL MEDICINE   (Hungary)

^d UNIVERSITY OF SYDNEY   (Australia)

^e KONKOLY OBSERVATORY   (Hungary)

Author keywords

Galaxies: individual: M 74; Stars: supernovae: individual: SN 2002ap

Indexed keywords

BAND STRUCTURE; CONTINUUM MECHANICS; KINETIC ENERGY; MATHEMATICAL MODELS; OPTICAL DEVICES; SPACE RESEARCH;

GAMMA-RAY BURSTS; INTRINSIC KINETIC ENERGY; SUPERNOVAE;

ASTROPHYSICS;

EID: 9144246339     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20040272     Document Type: Article

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