J/A+A/297/49 J/A+A/297/49 Supernovae spatial distribution A R Petrosian M Turatto Astron. Astrophys. 297 49 1995 1995A&A...297...49P galaxies: interactions galaxies: starburst supernovae: general In order to investigate the location of supernovae (SNe) in paired and interacting galaxies, the 54 supernovae discovered up to May 1993 in 14 Isolated Pairs of Galaxies and in 32 Interacting Systems were taken as a sample and studied.

Gal Galaxy name --- MType Galaxy type --- log(Lp/Ln) Logarithmic ratio of the blue luminosity of the SN parent galaxy to that of its close neighbour, corrected for galactic absorption --- alpha Far Infrared spectral index number=1 Computed via relation: {alpha}^100^_60_=log(S_{nu}_(100)/S_{nu}_(60)) /log(60/100), where S_{nu}_(100) and S_{nu}_(60) are the FIR flux densities at the wavelengths 60um and 100um, respectively. --- log(LFIR/Lb) Far infrared to B luminosity ratio --- D(V) Difference of the velocities of the parent and the neighbour galaxy, retrieved from the most recent literature km/s SN Supernova name --- SNType Supernova type --- theta Distance of the SN from the center of the galaxy in units of the galactic radius at 25 mag/arcsec^2^ --- theta0 Corrected value of theta for the tilting of the parent galaxies along the line of sight --- r/R1,2 Ratio of the projected distance of the SN from the parent galaxy nuclei to the projected separation between components of the paired/interacting galaxies --- PA Position angle of the SNE with respect to the neighbours number=2 The PA is computed clockwise with the companion placed at 180deg. deg Patricia Bauer CDS 1994Nov07 J_A+A_297_49.xml