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/journal_tables/A+AS/114/215/

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J/A+AS/114/215             New SNR candidates in M31    (Magnier+, 1995)
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New supernova remnant candidates in M31
     Magnier E.A., Prins S., van Paradijs J., Lewin W.H.G., Supper R.,
     Hasinger G., Pietsch W., Truemper J.
    <Astron. Astrophys. Suppl. Ser. 114, 215 (1995)>
    =1995A&AS..114..215M      (SIMBAD/NED BibCode)
================================================================================
ADC_Keywords: Supernova remnants ; H II regions
Keywords: galaxies: M31, ISM - ISM: supernova remnants, HII regions, bubbles

Description:
    We have performed a CCD H{alpha}, [SII], V survey of ~1.0 square
    degree of the disk of M 31 to search for new supernova remnant (SNR)
    candidates. We have identified candidates based on a combination of
    criteria: optical line-flux ratios, the presence or absence of
    ionizing blue stars, and optical morphology. We have identified a
    total of 178 candidate SNRs, divided into three confidence categories:
    13 with the highest confidence, 54 with moderate confidence, and 111
    with the lowest confidence. We have also identified 14 large
    structures with the characteristics of the superbubbles seen in the
    Galaxy and Magellanic Clouds. Of our 178 candidates, 15 have been
    identified in previous searches (Braun & Walterbos 1993; Blair et al.
    1981; D'Odorico et al. 1980). We present finding charts of all
    candidate SNRs and the superbubbles we have noted. We also present a
    detailed discussion of SNR searches in the Local Group.

File Summary:
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  FileName     Lrecl  Records   Explanations
--------------------------------------------------------------------------------
ReadMe            80        .   This file
table1            40       17   Image parameters
table2            92       19   O and early B stars and their Stroemgren spheres
table3            91       14   The superbubbles
table4           103       13   Our highest-confidence SNR candidates
table5           128       54   Our middle-confidence SNR candidates
table6           136      111   Our lowest-confidence SNR candidates
table7            89       55   SNR candidates from other authors not
                                 identified in our images
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Byte-by-byte Description of file: table1
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   Bytes Format    Units      Label     Explanations
--------------------------------------------------------------------------------
   1-  2  I2       ---        Field     Field number
       3  A1       ---      n_Field     [b] Note on field (1)
   5- 11  F7.4     deg        RAd       Right ascension (J2000.0)
  13- 19  F7.4     deg        DEd       Declination (J2000.0)
  21- 24  I4       s          ExpHa     Exposure time in H{alpha}
  26- 29  I4       s          ExpSII    Exposure time in [SII]
  31- 32  I2       s          ExpV      Exposure time in V
  34- 36  F3.1 10-16mW/m2/pix NoiseHa   ? Noise/pixel in H{alpha}
  38- 40  F3.1 10-16mW/m2/pix NoiseSII  ? Noise/pixel in [SII]
--------------------------------------------------------------------------------
Note (1): b: images not used in analysis
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Byte-by-byte Description of file: table2
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   Bytes Format  Units    Label   Explanations
--------------------------------------------------------------------------------
   1-  8  A8     ---      Sp      Spectral type
  10- 13  F4.1   mag      MVmag   Absolute V magnitude
  15- 18  F4.1   mag      Vmag    Apparent V magnitude
  20- 24  F5.2   mag      B-V     B-V colour index
  26- 30  F5.2   s-1   logN(Lyc)  Production rate of Lyman continuum photons
  32- 36  F5.2   10-7W logL(Ha)   Expected H{alpha} luminosity at the distance
                                   of M 31
  38- 43  F6.2   mW/m2 logF(Ha)   Expected H{alpha} flux at the distance of M 31
  45- 50  F6.3   pc/cm2   U       Excitation parameter for such photon rate
  52- 57  F6.3   pc       Rad     Stroemgren sphere radii for a
                                   ISM density n_H_=1cm^-3^
  59- 64  F6.3   cm-2  log(NH)    Hydrogen column density for n_H_=1cm^-3^
  66- 70  F5.3   mag      AV      Expected optical extinction for n_H_=1cm^-3^
  72- 76  F5.3   pc       Rad100  Stroemgren sphere radii for a
                                   ISM density n_H_=100cm^-3^
  78- 83  F6.3   cm-2  log(NH)100 Hydrogen column density for n_H_=100cm^-3^
  85- 89  F5.3   mag      AV100   Expected optical extinction for n_H_=100cm^-3^
      91  A1     ---      Note1   [*] * for HII regions detectable in our images
                                      (bold lines in printed table)
      92  A1     ---      Note2   [c] c for stars included in the completness
                                         limit of our blue star list
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Byte-by-byte Description of file: table3 table4 table5 table6
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   Bytes Format Units   Label     Explanations
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   2-  6  A5    ---     ID        Identification number
   8- 14  F7.4  deg     RAdeg     Right ascension (J2000)
  16- 22  F7.4  deg     DEdeg     Declination (J2000)
  24- 28  F5.1  arcsec  DeltaRA   Approximate extent of the object in
                                  right ascension
  30- 34  F5.1  arcsec  DeltaDE   Approximate extent of the object in
                                  declination
  36- 39  F4.1  arcsec  Diam      ? Diameter of the object
      40  A1    ---   n_Diam      When '*' extrapolated diameter
  45- 49  A5    ---     Pict      Picture number
  51- 52  A2    ---     Fig       Figure number (5a through 5m)
  54- 55  I2    ---     Field     Field number in which the candidate was
                                  identified
  57-137  A81   ---     Comments  Comments
--------------------------------------------------------------------------------

Byte-by-byte Description of file: table7
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   Bytes Format Units   Label     Explanations
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   2-  7  A6    ---     ID        SNR Identification
   9- 15  F7.4  deg     RAdeg     Right ascension (J2000)
  17- 23  F7.4  deg     DEdeg     Declination (J2000)
  25- 89  A65   ---     Comments  Comments
--------------------------------------------------------------------------------

References:
   Blair et al. 1981, ApJ 247, 879                 =1981ApJ...247..879B
   Braun R. and Walterbos R. 1993, A&AS 98, 327    =1993A&AS...98..327B
   D'Odorico S. et al. 1980, A&AS 40, 67           =1980A&AS...40...67D
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================================================================================
(End)                                          Simona Mei [CDS]   28-Sep-1995

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