Please use this identifier to cite or link to this item: http://hdl.handle.net/10995/101700
Title: Sub-arcsecond (Sub)millimeter Imaging of the Massive Protocluster G358.93-0.03: Discovery of 14 New Methanol Maser Lines Associated with a Hot Core
Authors: Brogan, C. L.
Hunter, T. R.
Towner, A. P. M.
McGuire, B. A.
MacLeod, G. C.
Gurwell, M. A.
Cyganowski, C. J.
Brand, J.
Burns, R. A.
O, Garatti, A. C.
Chen, X.
Chibueze, J. O.
Hirano, N.
Hirota, T.
Kim, K. -T.
Kramer, B. H.
Linz, H.
Menten, K. M.
Remijan, A.
Sanna, A.
Sobolev, A. M.
Sridharan, T. K.
Stecklum, B.
Sugiyama, K.
Surcis, G.
Van, Der, Walt, J.
Volvach, A. E.
Volvach, L. N.
Issue Date: 2019
Publisher: Institute of Physics Publishing
Citation: Sub-arcsecond (Sub)millimeter Imaging of the Massive Protocluster G358.93-0.03: Discovery of 14 New Methanol Maser Lines Associated with a Hot Core / C. L. Brogan, T. R. Hunter, A. P. M. Towner, et al. — DOI 10.3847/2041-8213/ab2f8a // Astrophysical Journal Letters. — 2019. — Vol. 881. — Iss. 2. — L39.
Abstract: We present (sub)millimeter imaging at 0.″5 resolution of the massive star-forming region G358.93-0.03 acquired in multiple epochs at 2 and 3 months following the recent flaring of its 6.7GHz CH3OH maser emission. Using the Submillimeter Array and Atacama Large Millimeter/submillimeter Array, we have discovered 14 new Class II CH3OH maser lines ranging in frequency from 199 to 361 GHz, which originate mostly from=1 torsionally excited transitions and include one=2 transition. The latter detection provides the first observational evidence that Class II maser pumping involves levels in the=2 state. The masers are associated with the brightest continuum source (MM1), which hosts a line-rich hot core. The masers present a consistent curvilinear spatial velocity pattern that wraps around MM1, suggestive of a coherent physical structure 1200 au in extent. In contrast, the thermal lines exhibit a linear pattern that crosses MM1 but at progressive position angles that appear to be a function of either increasing temperature or decreasing optical depth. The maser spectral profiles evolved significantly over one month, and the intensities dropped by factors of 3.0-7.2, with the=2 line showing the largest change. A small area of maser emission from only the highest excitation lines closest to MM1 has disappeared. There are seven additional dust continuum sources in the protocluster, including another hot core (MM3). We do not find evidence for a significant change in (sub)millimeter continuum emission from any of the sources during the one month interval, and the total protocluster emission remains comparable to prior single-dish measurements. © 2019. The American Astronomical Society. All rights reserved..
Keywords: ISM: INDIVIDUAL OBJECTS (G358.93-0.03)
MASERS
STARS: FORMATION
STARS: PROTOSTARS
URI: http://hdl.handle.net/10995/101700
Access: info:eu-repo/semantics/openAccess
SCOPUS ID: 85072604216
PURE ID: 10497434
ISSN: 20418205
DOI: 10.3847/2041-8213/ab2f8a
Appears in Collections:Научные публикации, проиндексированные в SCOPUS и WoS CC

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