Molecular line search towards the flaring 6.7-GHz methanol masers of G 24.33+0.13 and G 359.62−0.24: rare maser transitions detected

Author:

McCarthy T P1ORCID,Orosz G1,Ellingsen S P1ORCID,Breen S L2ORCID,Voronkov M A3,Burns R A45,Olech M6,Yonekura Y7,Hirota T48,Hyland L J1,Wolak P9

Affiliation:

1. School of Natural Sciences, University of Tasmania, Private Bag 37, Hobart, Tasmania, NSW 7001, Australia

2. SKAO, Jodrell Bank, Lower Withington, Macclesfield, Cheshire SK11 9FT, UK

3. CSIRO Space and Astronomy, PO Box 76, Epping, NSW 2121, Australia

4. Mizusawa VLBI Observatory, National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan

5. Korea Astronomy and Space Science Institute, 776 Daedeokdae-ro, Yuseong-gu, Daejeon 34055, Republic of Korea

6. Space Radio-Diagnostics Research Centre, University of Warmia and Mazury, ul.Oczapowskiego 2, PL-10-719 Olsztyn, Poland

7. Center for Astronomy, Ibaraki University, 2-1-1 Bunkyo, Mito, Ibaraki 310-8512, Japan

8. Department of Astronomical Sciences, SOKENDAI (The Graduate University for Advanced Studies), Osawa 2-21-1, Mitaka-shi, Tokyo 181-8588, Japan

9. Institute of Astronomy, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University, Grudziadzka 5, PL-87-100 Torun, Poland

Abstract

ABSTRACT We have performed a molecular line search towards the flaring 6.7-GHz masers G 24.33+0.13, and G 359.6−0.24 using the Australia Telescope Compact Array. We present spectra of the 6.7-GHz class II methanol and 22.2-GHz water masers towards these sources and provide a comparison with other recent flaring events these sources have experienced. We also detect the fourth example of a 23.4-GHz class I methanol maser and the 11th example of a 4.8-GHz formaldehyde maser towards G 24.33+0.13. Alongside these results, we also observe the previously detected ammonia (3,3) emission and report upper limits on the presence of various other cm-wavelength methanol, ammonia, and OH transitions. Our results are consistent with the flaring of G 24.33+0.13 being driven by a variable accretion rate in the host high mass young stellar object.

Funder

Ministry of Education and Science

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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