Oxygen recombination in the nebular phase of supernovae 1998bw and 2002ap

Monthly Notices of the Royal Astronomical Society

Volumn 408, Issue 2, 2010, Pages 947-960

  Maurer, I ^a   Mazzali, P A ^a,b,c  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b SCUOLA NORMALE SUPERIORE   (Italy)

^c National Institute for Astrophysics OAPd   (Italy)

Author keywords

Line: formation; Radiation mechanisms: non thermal; Radiative transfer; Supernovae: general

Indexed keywords

EMISSION SPECTROSCOPY; EXCITED STATES; GROUND STATE; THERMIONIC EMISSION;

ATOMIC DATA; CORE COLLAPSE SUPERNOVAE; ELECTRON EXCITATIONS; LINE FORMATIONS; OXYGEN RECOMBINATION; RADIATION MECHANISMS: NONTHERMAL; SUPERNOVAE: GENERAL; TEMPERATURE DEPENDENT; THERMAL ELECTRON; TIME SPECTRUM;

SUPERNOVAE;

EID: 78649436431     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.17096.x     Document Type: Article

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