Multi-wavelength maser observations of the Extended Green Object G19.01—0.03

  • Gwenllian M. Williams
  • , Claudia J. Cyganowski
  • , Crystal L. Brogan
  • , Todd R. Hunter
  • , John D. Ilee
  • , Pooneh Nazari
  • , Rowan J. Smith

Research output: Contribution to journalArticlepeer-review

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Abstract

We report the detections of NH3(3,3) and 25 GHz and 278.3 GHz class I CH3OH maser emission associated with the outflow of the Extended Green Object G19.01-0.03 in sub-arcsecond resolution Atacama Large Millimeter/submillimeter Array (ALMA) and Karl G. Jansky Very Large Array (VLA) observations. For masers associated with the outer outflow lobes (> 12.5 ″ from the central massive young stellar object; MYSO), the spatial distribution of the NH3(3,3) masers is statistically indistinguishable from that of previously known 44 GHz Class I CH3OH masers, strengthening the connection of NH3(3,3) masers to outflow shocks. In sub-arcsecond resolution VLA observations, we resolve the 6.7 GHz Class II CH3OH maser emission towards the MYSO into a partial, inclined ring, with a velocity gradient consistent with the rotationally supported circumstellar disc traced by thermal gas emission.
Original languageEnglish
Pages (from-to)261-263
Number of pages3
JournalProceedings of the International Astronomical Union
Volume18
DOIs
Publication statusPublished - 07 Feb 2024
Externally publishedYes

Keywords

  • masers
  • stars: formation
  • stars: individual: G19.01-0.03
  • stars: massive
  • stars: protostars
  • techniques: interferometric

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