Eales, SA;
              
      
            
                Smith, MWL;
              
      
            
                Wilson, CD;
              
      
            
                Bendo, GJ;
              
      
            
                Cortese, L;
              
      
            
                Pohlen, M;
              
      
            
                Boselli, A;
              
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
            ... Zeilinger, WW; + view all
            
          
      
        
        
        
    
  
(2010)
  Mapping the interstellar medium in galaxies with Herschel/SPIRE*.
Astronomy & Astrophysics
, 518
      
    
    
    
    , Article L62.     10.1051/0004-6361/201014536.
  
  
      
    
  
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Abstract
The standard method of mapping the interstellar medium in a galaxy, by observing the molecular gas in the CO 1-0 line and the atomic gas in the 21-cm line, is largely limited with current telescopes to galaxies in the nearby universe. In this letter, we use SPIRE observations of the galaxies M 99 and M 100 to explore the alternative approach of mapping the interstellar medium using the continuum emission from the dust. We have compared the methods by measuring the relationship between the star-formation rate and the surface density of gas in the galaxies using both methods. We find the two methods give relationships with a similar dispersion, confirming that observing the continuum emission from the dust is a promising method of mapping the interstellar medium in galaxies.
| Type: | Article | 
|---|---|
| Title: | Mapping the interstellar medium in galaxies with Herschel/SPIRE* | 
| Open access status: | An open access version is available from UCL Discovery | 
| DOI: | 10.1051/0004-6361/201014536 | 
| Publisher version: | https://doi.org/10.1051/0004-6361/201014536 | 
| Language: | English | 
| Additional information: | This version is the version of record. For information on re-use, please refer to the publisher’s terms and conditions. | 
| Keywords: | galaxies: ISM / galaxies: spiral / dust, extinction / ISM: abundances | 
| UCL classification: | UCL UCL > Provost and Vice Provost Offices > UCL BEAMS UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics  | 
        
| URI: | https://discovery.ucl.ac.uk/id/eprint/10095314 | 
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