A CATALOG OF CH3OH 70-61A+ MASER SOURCES IN MASSIVE STAR-FORMING REGIONS. II. MASERS IN NGC 6334F, G8.67-0.36, AND M17

被引：12

作者：

Gomez, Laura ^{[1
,2
]}

Luis, Leticia ^{[2
]}

Hernandez-Curiel, Idalia ^{[2
,3
]}

Kurtz, Stan E. ^{[2
]}

Hofner, Peter ^{[4
,5
]}

Araya, Esteban D. ^{[6
]}

机构：

[1] Max Planck Inst Radioastron, D-53121 Bonn, Germany

[2] UNAM, Ctr Radioastron & Astrofis, Morelia 58090, Michoacan, Mexico

[3] Inst Nacl Astrofis Opt & Electr, Puebla 72840, Mexico

[4] New Mexico Inst Min & Technol, Dept Phys, Socorro, NM 87801 USA

[5] Natl Radio Astron Observ, Socorro, NM 87801 USA

[6] Western Illinois Univ, Dept Phys, Macomb, IL 61455 USA

来源：

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2010年 / 191卷 / 02期

基金：

美国国家科学基金会;

关键词：

H II regions; ISM: individual objects (NGC 6334F; G8.67-0.36; M17); masers; stars: formation; GHZ METHANOL MASERS; ULTRACOMPACT HII-REGIONS; CLASS-I; VLBI OBSERVATIONS; NGC-6334; OH; MORPHOLOGIES; OUTFLOW; GLIMPSE; OBJECTS;

D O I：

10.1088/0067-0049/191/2/207

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present Very Large Array (VLA) observations of the 7(0)-6(1)A(+) methanol maser transition at 44 GHz toward NGC 6334F, G8.67-0.36, and M17. These arcsecond resolution observations complete a previous, larger VLA survey of this maser transition in high-mass, star-forming regions reported by Kurtz et al. We confirm the presence of 44 GHz methanol maser emission in all 3 sources, detecting 8 distinct maser components in NGC 6334F, 12 components in G8.67-0.36, and 1 in M17.

引用

页码：207 / 211

页数：5

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