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The protostellar mass limit for 6.7 GHz methanol masers I. A low-mass YSO survey

Citation

Minier, V and Ellingsen, SP and Norris, RP and Booth, RS, The protostellar mass limit for 6.7 GHz methanol masers I. A low-mass YSO survey, Astronomy & Astrophysics, 403, (3) pp. 1095-1100. ISSN 0004-6361 (2003) [Refereed Article]

DOI: doi:10.1051/0004-6361:20030465

Abstract

We report the results of a search for 6.7 GHz methanol masers toward low-mass young stellar objects (YSOs) and (pre)protostellar condensations with the Australia Telescope Compact Array (ATCA). Our sample consisted of 13 class 0 protostars and 44 class I YSOs as well as 66 (pre)protostellar condensations. A single detection was obtained toward NGC 2024: FIR4 in the Orion B region. This is the first detection of a 6.7 GHz methanol maser in Orion. The nature of FIR4 has been a subject of debate with some evidence suggesting that it is a very cold high-mass (pre)protostellar condensation and others arguing that it is a low-mass YSO. The discovery of a methanol maser associated with this source is inconsistent with both of these hypotheses and we suggest that FIR4 probably harbours an intermediate- or high-mass YSO. The less massive objects in our sample do not exhibit any methanol maser stronger than 400 mJy (4σ). Based on the nil detection rate toward the low-mass YSOs we can place an upper limit of 3 × 106 K on the brightness temperature of any methanol maser associated with class 0.I or II sources. These results support the hypothesis that no strong methanol masers are associated with low-mass star formation (≲ 3 M⊙).

Item Details

Item Type:Refereed Article
Research Division:Physical Sciences
Research Group:Astronomical and Space Sciences
Research Field:Galactic Astronomy
Objective Division:Expanding Knowledge
Objective Group:Expanding Knowledge
Objective Field:Expanding Knowledge in the Physical Sciences
Author:Ellingsen, SP (Professor Simon Ellingsen)
ID Code:28534
Year Published:2003
Web of Science® Times Cited:130
Deposited By:Physics
Deposited On:2003-08-01
Last Modified:2004-04-07
Downloads:0

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