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A study of methanol masers at 36 and 44 GHz and 48 GHz thermal emission around them

  • S. V. Kalenskii
  • I. I. Berulis
  • I. E. Val'tts
  • V. I. Slysh
  • R. Bachiller
  • J. Gomez-Gonzalez
  • J. Martin-Pintado
  • A. Rodriguez-Franco
8. Methanol Masers in Star Forming Regions
Part of the Lecture Notes in Physics book series (LNP, volume 412)

Abstract

An extensive search for new methanol sources were made. Three new masers in the 70-61A+ transition and twenty-four new thermal sources in the 10−00A+ transition were detected. Our results support the idea that high- velocity flows may increase the abundance of methanol and that methanol masers arise in methanol-rich sources.

Keywords

Radio Telescope Velocity Outflow Methanol Maser IRAS Source Dust Envelope 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

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Copyright information

© Springer-Verlag 1993

Authors and Affiliations

  • S. V. Kalenskii
    • 1
  • I. I. Berulis
    • 1
  • I. E. Val'tts
    • 1
  • V. I. Slysh
    • 1
  • R. Bachiller
    • 2
  • J. Gomez-Gonzalez
    • 2
  • J. Martin-Pintado
    • 2
  • A. Rodriguez-Franco
    • 2
  1. 1.Astro Space CenterMoscow
  2. 2.Centro Astronomico de YebesGuadalajara

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