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Evidence for an Interaction between the Galactic Center Clouds M0.10-0.08 and M0.11-0.11
Journal article   Open access   Peer reviewed

Evidence for an Interaction between the Galactic Center Clouds M0.10-0.08 and M0.11-0.11

Natalie O. Butterfield, Cornelia C. Lang, Adam Ginsburg, Mark R. Morris, Juergen Ott and Dominic A. Ludovici
The Astrophysical journal, Vol.936(2), p.186
09/01/2022
DOI: 10.3847/1538-4357/ac887c
url
https://doi.org/10.3847/1538-4357/ac887cView
Published (Version of record) Open Access

Abstract

We present high-resolution (similar to 2-3 ''; similar to 0.1 pc) radio observations of the Galactic center cloud M0.10-0.08 using the Very Large Array at K and Ka band (similar to 25 and 36 GHz). The M0.10-0.08 cloud is located in a complex environment near the Galactic center Radio Arc and the adjacent M0.11-0.11 molecular cloud. From our data, M0.10-0.08 appears to be a compact molecular cloud (similar to 3 pc) that contains multiple compact molecular cores (5+; <0.4 pc). In this study, we detect a total of 15 molecular transitions in M0.10-0.08 from the following molecules: NH3, HC3N, CH3OH, HC5N, CH3CN, and OCS. We have identified more than sixty 36 GHz CH3OH masers in M0.10-0.08 with brightness temperatures above 400 K and 31 maser candidates with temperatures between 100 and 400 K. We conduct a kinematic analysis of the gas using NH3 and detect multiple velocity components toward this region of the Galactic center. The bulk of the gas in this region has a velocity of 51.5 km s(-1) (M0.10-0.08) with a lower-velocity wing at 37.6 km s(-1). We also detect a relatively faint velocity component at 10.6 km s(-1) that we attribute to being an extension of the M0.11-0.11 cloud. Analysis of the gas kinematics, combined with past X-ray fluorescence observations, suggests M0.10-0.08 and M0.11-0.11 are located in the same vicinity of the Galactic center and could be physically interacting.
Astronomy & Astrophysics Physical Sciences Science & Technology

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