Interpretation of the Early Spectra of SN 1993J in M81

view Abstract Citations (41) References (10) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Interpretation of the Early Spectra of SN 1993J in M81 Baron, E. ; Hauschildt, P. H. ; Branch, D. ; Wagner, R. M. ; Austin, S. J. ; Filippenko, A. V. ; Matheson, T. Abstract We present optical spectra obtained on 1993 April 7 and April 13 of the bright supernova SN 1993J in the nearby galaxy M81. The spectra show strong hydrogen Balmer lines with pronounced P Cygni profiles, except for Hα, which is greatly dominated by emission. In order to obtain diagnostics on the velocities, temperatures, densities, and composition of the atmosphere, we present non-local thermodynamic equilibrium (NLTE) synthetic spectrum fits to these observations. For April 7 we find a photospheric velocity of 10,000-11,000 km s^-1^, with a photospheric electron temperature of 7500-8000 K and a radius of 10^15^ cm. On April 13 the photospheric velocity is about 11,000 km s^-1^, the photospheric temperature is about 6500 K, and the radius is ~1.6 x 10^15^ cm. Most of the features of the spectra are well fitted by model atmospheres with solar composition. We find a distance for SN 1993J of 4.0 +/- 0.5 Mpc and the explosion epoch to be UT 1993 March 27.5+/-0.5. Publication: The Astrophysical Journal Pub Date: October 1993 DOI: 10.1086/187061 Bibcode: 1993ApJ...416L..21B Keywords: STARS: SUPERNOVAE: INDIVIDUAL ALPHANUMERIC: SN 1993J full text sources ADS | data products SIMBAD (2) NED (2)