Please use this identifier to cite or link to this item: http://hdl.handle.net/10995/102084
Title: 13CH3OH Masers Associated with a Transient Phenomenon in a High-mass Young Stellar Object
Authors: Chen, X.
Sobolev, A. M.
Breen, S. L.
Shen, Z. -Q.
Ellingsen, S. P.
MacLeod, G. C.
Li, B.
Voronkov, M. A.
Kaczmarek, J. F.
Zhang, J.
Ren, Z. -Y.
Wang, J.
Linz, H.
Hunter, T. R.
Brogan, C.
Sugiyama, K.
Burns, R. A.
Menten, K.
Sanna, A.
Stecklum, B.
Hirota, T.
Kim, K. -T.
Chibueze, J.
Heever, S. P. V. D.
Issue Date: 2020
Publisher: Institute of Physics Publishing
Citation: 13CH3OH Masers Associated with a Transient Phenomenon in a High-mass Young Stellar Object / X. Chen, A. M. Sobolev, S. L. Breen, et al. — DOI 10.3847/2041-8213/ab72a5 // Astrophysical Journal Letters. — 2020. — Vol. 890. — Iss. 2. — L22.
Abstract: We report the first detection of isotopic methanol (13CH3OH) maser emission in interstellar space. The emission was detected toward the high-mass young stellar object G358.93-0.03 during monitoring of a flare in the 6.7 GHz methanol (CH3OH) maser emission in this source. We find that the spectral and spatial distribution of the 13CH3OH masers differs from the CH3OH masers imaged at the same epoch, contrary to expectations from similarity of their pumping. This conclusively demonstrates that isotopic methanol masers are bright under different physical conditions and suggests that they can provide additional, complementary information to the CH3OH masers from the same source. We detect a rapid decay of the 13CH3OH maser lines suggesting that they are transient phenomena (masing for only a few months), likely associated with rapid changes in radiation field due to an accretion burst induced by massive disk fragmentation. Changes in the line flux density are faster than required to achieve equilibrium in the energy level populations, indicating that the pumping of these masers is likely variable. © 2020. The American Astronomical Society. All rights reserved..
URI: http://hdl.handle.net/10995/102084
Access: info:eu-repo/semantics/openAccess
SCOPUS ID: 85081694063
PURE ID: 12435892
876d54cd-4b68-4175-9f8a-37c38de1b7e5
ISSN: 20418205
DOI: 10.3847/2041-8213/ab72a5
Appears in Collections:Научные публикации, проиндексированные в SCOPUS и WoS CC

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