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J/A+A/297/49        Supernovae spatial distribution           (Petrosian+, 1995)

The spatial distribution of supernovae in paired and interacting galaxies PETROSIAN A.R., TURATTO M. <Astron. Astrophys. 297, 49 (1995)> =1995A&A...297...49P (SIMBAD/NED Reference)
ADC_Keywords: Supernovae; Stellar distribution Keywords: galaxies: interaction - galaxies: starburst - supernovae: general Description: 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. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1 80 74 Interacting galaxies with supernovae table2 80 29 Isolated Pairs of galaxies with Supernovae
Byte-by-byte Description of file: table1 table2
Bytes Format Units Label Explanations
1- 18 A18 --- Gal Galaxy name 20- 25 A6 --- MType Galaxy type 27- 31 F5.2 --- log(Lp/Ln) []? Logarithmic ratio of the blue luminosity of the SN parent galaxy to that of its close neighbour, corrected for galactic absorption 33- 37 F5.2 --- alpha []? Far Infrared spectral index (1) 39- 43 F5.2 --- log(LFIR/Lb) []? Far infrared to B luminosity ratio 45- 49 I5 km/s D(V) []? Difference of the velocities of the parent and the neighbour galaxy, retrieved from the most recent literature 51- 56 A6 --- SN Supernova name 58- 60 A3 --- SNType Supernova type 62- 65 F4.2 --- theta []? Distance of the SN from the center of the galaxy in units of the galactic radius at 25 mag/arcsec2 67- 70 F4.2 --- theta0 []? Corrected value of theta for the tilting of the parent galaxies along the line of sight 72- 76 F5.3 --- 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 78- 80 I3 deg PA []? Position angle of the SNE with respect to the neighbours (2)
Note (1): Computed via relation: α10060=log(Sν(100)/Sν(60)) /log(60/100), where Sν(100) and Sν(60) are the FIR flux densities at the wavelengths 60um and 100um, respectively. Note (2): The PA is computed clockwise with the companion placed at 180deg.

(End) Patricia Bauer [CDS] 07-Nov-1994
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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