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D.M. Cragg

Identifiers

  • name variant D.M. Cragg 0.60 · backfill

Papers (4)

  1. How do methanol masers manage to appear in the youngest star vicinities and isolated molecular clumps? astro-ph · 2007 · author #2
  2. Model of the W3(OH) environment based on data for both maser and 'quasi-thermal' methanol lines astro-ph · 2004 · author #3
  3. Discovery of new 19.9-GHz methanol masers in star forming regions astro-ph · 2004 · author #2
  4. Masers and Outflows in the W3(OH)/W3(H2O) region astro-ph · 2004 · author #3

Mentions

  • 0706.3117 #2 · backfill · confidence 0.70 D.M. Cragg

Frequent Coauthors