J/A+A/462/81        L_IR_-T_dust_ relation in galaxies       (Chanial+, 2007)
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The infrared compactness-temperature relation for quiescent and starburst
galaxies.
    Chanial P., Flores H., Guiderdoni B., Elbaz D., Hammer F., Vigroux L.
   <Astron. Astrophys., 462, 81-91 (2007)>
   =2007A&A...462...81C
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ADC_Keywords: Galaxies, radio ; Galaxies, IR ; Effective temperatures
Keywords: galaxies: fundamental parameters - galaxies: starburst -
          infrared: galaxies - radio continuum: galaxies

Abstract:
    IRAS observations show the existence of a correlation between the
    infrared luminosity L_IR_ and dust temperature T_d_ in star-forming
    galaxies, in which larger L_IR_ leads to higher dust temperature. The
    L_IR_-T_d_ relation is commonly seen as reflecting the increase in
    dust temperature in galaxies with higher star formation rate (SFR).
    Even though the correlation shows a significant amount of dispersion,
    a unique relation has been commonly used to construct spectral energy
    distributions (SEDs) of galaxies in distant universe studies, such as
    source number counting or photometric redshift determination.
    In this work, we introduce a new parameter, namely the size of the
    star-forming region r_IR_ and lay out the empirical and modelled
    relation between the global parameters L_IR_, T_d_ and r_IR_ of
    IR-bright non-AGN galaxies.

File Summary:
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 FileName    Lrecl  Records   Explanations
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ReadMe          80        .   This file
table4.dat      95      134   Global properties of the 170um sample resolved in
                               the NVSS (Cat. <VIII/65>) radio continuum catalog
table5.dat      95       64   Global properties of the 170um sample resolved in
                               the FIRST (Cat. <VII/71>) radio continuum catalog
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See also:
   VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998)
   VIII/71 : The FIRST Survey Catalog, Version 03Apr11 (Becker+ 2003)

Byte-by-byte Description of file: table[45].dat
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   Bytes Format Units       Label     Explanations
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   1- 23  A23   ---         Name      Source name
  25- 31  I7    ---         PGC       PGC number
  33- 34  I2    h           RAh       Right ascension (J2000)
  36- 37  I2    min         RAm       Right ascension (J2000)
  39- 43  F5.2  s           RAs       Right ascension (J2000)
      45  A1    ---         DE-       Declination sign (J2000)
  46- 47  I2    deg         DEd       Declination (J2000)
  49- 50  I2    arcmin      DEm       Declination (J2000)
  52- 55  F4.1  arcsec      DEs       Declination (J2000)
  57- 60  A4    ---         MType     Morphological type from HYPERLEDA
  63- 67  F5.1  Mpc         Dist      Distance
  70- 74  F5.2 [solLum]     logLIR    Infrared luminosity (1)
  76- 80  F5.2  ---         logLIR/LB ? Ratio of the IR to B-band luminosities
  82- 85  F4.2  [pc]        logrIR    IR physical radius
  87- 90  F4.2 [solLum/pc2] logSIR    IR surface brightness
  92- 95  F4.1  K           Td        Effective dust temperature
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Note (1): Infrared luminosity derived from the 60 and 100 flux densities, 
          by assuming a modified blackbody of emissivity index {beta}=1.3
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History:
    From electronic version of the journal
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(End)                                      Patricia Vannier [CDS]    10-Sep-2007
