Nebular emission-line profiles of Type Ib/c supernovae - Probing the ejecta asphericity

Monthly Notices of the Royal Astronomical Society

Volumn 397, Issue 2, 2009, Pages 677-694

  Taubenberger, S ^a   Valenti, S ^b,c   Benetti, S ^d   Cappellaro, E ^d   Della Valle, M ^e   Elias Rosa, N ^a,f   Hachinger, S ^a   Hillebrandt, W ^a   Maeda, K ^a,g   Mazzali, P A ^a,d   Pastorello, A ^c   Patat, F ^b   Sim, S A ^a   Turatto, M ^h  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^c QUEEN'S UNIVERSITY BELFAST   (United Kingdom)

^d INAF OSSERVATORIO ASTRONOMICO DI PADOVA   (Italy)

^e INAF OSSERVATORIO ASTRONOMICO DI CAPODIMONTE   (Italy)

^f CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^g UNIVERSITY OF TOKYO   (Japan)

^h INAF OSSERVATORIO ASTROFISICO DI CATANIA   (Italy)

Author keywords

Line: profiles; Supernovae: general; Techniques: spectroscopic

Indexed keywords

ATMOSPHERIC OPTICS; GEOMETRY; MAGNESIUM COMPOUNDS; SUPERNOVAE;

ASPHERICITY; CORE COLLAPSE SUPERNOVAE; EMISSION LINES; FULL WIDTHS AT HALF MAXIMUMS; GAUSSIANS; LINE: PROFILES; SPECTRA'S; SUPERNOVAE: GENERAL; TECHNIQUES: SPECTROSCOPIC; TIME SPECTRUM;

GAUSSIAN DISTRIBUTION;

EID: 67651092142     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.15003.x     Document Type: Article

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