Star formation sites toward the Galactic center region: The correlation of CH 3 OH masers, H 2 O masers, and near-IR green sources

E. T. Chambers, F. Yusef-Zadeh, J. Ott

Research output: Contribution to journalArticlepeer-review

2 Scopus citations

Abstract

We present a study of star formation in the central molecular zone (CMZ) of our Galaxy through the association of three star formation indicators: 6.7 GHz CH3OH masers, 22 GHz H2O masers, and enhanced 4.5 μm emission ('green') sources. We explore how star formation in the CMZ(|ℓ| < 1.3, |b| < 10′) compares with that of the Galactic disk (6 > ℓ > 345, |b| < 2). Methods. Using an automated algorithm, we search for green sources toward 6.7 GHz CH3OH masers detected in the Parkes Methanol Multibeam Survey. We combine these results with lists of 22 GHz H 2O masers, including our Mopra survey of the CMZ. Results. We find that the correlation of CH3OH masers with green sources is a function of Galactic latitude, with a minimum close to b = 0 and increasing with |b| (toward the central part of the Galaxy, 6 > ℓ > 345, |b| < 2). We find no significant difference between the correlation rate of CH3OH masers with green sources in the CMZ and the disk. This suggests that although the physical conditions of the gas are different in the CMZ from that of the Galactic disk, once gravitational instability sets in at sufficiently high densities, signatures of star formation appear to be similar in both regions. Moreover, the detection of green sources, even at the distance of the Galactic center, shows that our technique can easily identify the early stages of star formation, especially in low-extinction regions of the Galaxy. Through the association of H2O and CH3OH masers, we identify 15 star-forming sites in the CMZ. We find a higher correlation rate of coincident H2O and CH3OH masers within the CMZ compared to the Galactic disk, indicating a difference in the maser evolutionary sequence for star-forming cores in these two regions.

Original languageEnglish (US)
Article number81
JournalAstronomy and Astrophysics
Volume563
DOIs
StatePublished - Mar 2014

Keywords

  • Galaxy: center
  • ISM: clouds
  • ISM: molecules
  • Stars: formation

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint Dive into the research topics of 'Star formation sites toward the Galactic center region: The correlation of CH <sub>3</sub> OH masers, H <sub>2</sub> O masers, and near-IR green sources'. Together they form a unique fingerprint.

Cite this