Improved distance determination to M 51 from supernovae 2011dh and 2005cs

Astronomy and Astrophysics

Volumn 540, Issue , 2012, Pages

  Vinko J ^a,c   Takats K ^a   Szalai, T ^a   Marion, G H ^b   Wheeler, J C ^c   Sarneczky K ^d   Garnavich, P M ^e   Kelemen, J ^d   Klagyivik, P ^d   Pal A ^d,f   Szalai, N ^d   Vida, K ^d  

^a UNIVERSITY OF SZEGED   (Hungary)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c The University of Texas at Austin   (United States)

^d INSTITUTE OF EXPERIMENTAL MEDICINE   (Hungary)

^e UNIVERSITY OF NOTRE DAME   (United States)

^f EÖTVÖS LORÁND UNIVERSITY   (Hungary)

Author keywords

galaxies: distances and redshifts; galaxies: individual: m 51; supernovae: individual: 2005cs; supernovae: individual: 2011dh

Indexed keywords

CORRECTION FACTORS; GALAXIES: DISTANCES AND REDSHIFTS; GALAXIES: INDIVIDUAL: M 51; H-CONTENT; HOST GALAXIES; IMPROVED DISTANCE; PHOTOSPHERE-METHODS; STANDARD TYPE; STELLAR CLUSTER; SUPERNOVAE: INDIVIDUAL;

GALAXIES;

STARS;

EID: 84859337966     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201118364     Document Type: Article

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