A 95 GHz methanol emission survey toward eight small supernova remnants

We report on a 95 GHz（80-71A＋） methanol（CH3OH） emission survey with the Purple Mountain Observatory Delingha 13.7 m telescope. Eight supernova remnants（SNRs） with angular size〈10′ were observed, but emission was only detected in three SNRs near the Galactic center（Sgr A East,G 0.1–0.1 and G 359.92–0...

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Published inResearch in astronomy and astrophysics Vol. 17; no. 12; pp. 65 - 76
Main Authors Li, Ying-Jie, Xu, Ye, Chen, Xi, Lu, Deng-Rong, Sun, Yan, Du, Xin-Yu, Shen, Zhi-Qiang
Format Journal Article
LanguageEnglish
Published Beijing National Astronomical Observatories, CAS and IOP Publishing Ltd 01.12.2017
IOP Publishing
Subjects
Emission
Galaxy: center
ISM: clouds
ISM: kinematics and dynamics
ISM: molecules
ISM: supernova remnants
Methanol
Molecular gases
Mountains
Polls & surveys
Star & galaxy formation
Star formation
Supernova
Supernova remnants
Online AccessGet full text
ISSN1674-4527
2397-6209
DOI10.1088/1674-4527/17/12/125

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Abstract We report on a 95 GHz（80-71A＋） methanol（CH3OH） emission survey with the Purple Mountain Observatory Delingha 13.7 m telescope. Eight supernova remnants（SNRs） with angular size〈10′ were observed, but emission was only detected in three SNRs near the Galactic center（Sgr A East,G 0.1–0.1 and G 359.92–0.09）. CH3OH emission mainly surrounds the SNRs and can be decomposed into nine spatial peaks with the velocity range of eight peaks being（-30, 70） km s-1, and the other is（70, 120） km s-1. They are probably excited by interaction with these SNRs and adjacent molecular gas in the central molecular zone（CMZ）, although star formation may play an important role in exciting CH3OH emission in some regions of CMZ. We infer that tidal action is unlikely to be an excitation source for CH3OH emission.
AbstractList We report on a 95 GHz ( 8 0 − 7 1 A+) methanol (CH3OH) emission survey with the Purple Mountain Observatory Delingha 13.7 m telescope. Eight supernova remnants (SNRs) with angular size ≲ 10 ′ were observed, but emission was only detected in three SNRs near the Galactic center (Sgr A East, G 0.1-0.1 and G 359.92-0.09). CH3OH emission mainly surrounds the SNRs and can be decomposed into nine spatial peaks with the velocity range of eight peaks being (−30, 70) km s−1, and the other is (70, 120) km s−1. They are probably excited by interaction with these SNRs and adjacent molecular gas in the central molecular zone (CMZ), although star formation may play an important role in exciting CH3OH emission in some regions of CMZ. We infer that tidal action is unlikely to be an excitation source for CH3OH emission.
We report on a 95 GHz (\({8}_{0}-{7}_{1}\) A+) methanol (CH3OH) emission survey with the Purple Mountain Observatory Delingha 13.7 m telescope. Eight supernova remnants (SNRs) with angular size \(\lesssim {10}^{^{\prime} }\) were observed, but emission was only detected in three SNRs near the Galactic center (Sgr A East, G 0.1–0.1 and G 359.92–0.09). CH3OH emission mainly surrounds the SNRs and can be decomposed into nine spatial peaks with the velocity range of eight peaks being (−30, 70) km s−1, and the other is (70, 120) km s−1. They are probably excited by interaction with these SNRs and adjacent molecular gas in the central molecular zone (CMZ), although star formation may play an important role in exciting CH3OH emission in some regions of CMZ. We infer that tidal action is unlikely to be an excitation source for CH3OH emission.
We report on a 95 GHz（80-71A＋） methanol（CH3OH） emission survey with the Purple Mountain Observatory Delingha 13.7 m telescope. Eight supernova remnants（SNRs） with angular size〈10′ were observed, but emission was only detected in three SNRs near the Galactic center（Sgr A East,G 0.1–0.1 and G 359.92–0.09）. CH3OH emission mainly surrounds the SNRs and can be decomposed into nine spatial peaks with the velocity range of eight peaks being（-30, 70） km s-1, and the other is（70, 120） km s-1. They are probably excited by interaction with these SNRs and adjacent molecular gas in the central molecular zone（CMZ）, although star formation may play an important role in exciting CH3OH emission in some regions of CMZ. We infer that tidal action is unlikely to be an excitation source for CH3OH emission.
Author Ying-Jie Li;Ye Xu;Xi Chen;Deng-Rong Lu;Yan Sun;Xin-Yu Du;Zhi-Qiang Shen
AuthorAffiliation Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China;University of Science and Technology of China, Chinese Academy of Sciences, Hefei 230026, China;Center for Astrophysics, Guangzhou University, Guangzhou 51006, China;Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China;University of the Chinese Academy of Sciences, Beijing 100049, China
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ISM：molecules;ISM：supernova remnants;Galaxy：center;ISM：kinematics and dynamics;ISM：clouds
We report on a 95 GHz（80-71A＋） methanol（CH3OH） emission survey with the Purple Mountain Observatory Delingha 13.7 m telescope. Eight supernova remnants（SNRs） with angular size〈10′ were observed, but emission was only detected in three SNRs near the Galactic center（Sgr A East,G 0.1–0.1 and G 359.92–0.09）. CH3OH emission mainly surrounds the SNRs and can be decomposed into nine spatial peaks with the velocity range of eight peaks being（-30, 70） km s-1, and the other is（70, 120） km s-1. They are probably excited by interaction with these SNRs and adjacent molecular gas in the central molecular zone（CMZ）, although star formation may play an important role in exciting CH3OH emission in some regions of CMZ. We infer that tidal action is unlikely to be an excitation source for CH3OH emission.
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Snippet We report on a 95 GHz（80-71A＋） methanol（CH3OH） emission survey with the Purple Mountain Observatory Delingha 13.7 m telescope. Eight supernova remnants（SNRs）...
We report on a 95 GHz ( 8 0 − 7 1 A+) methanol (CH3OH) emission survey with the Purple Mountain Observatory Delingha 13.7 m telescope. Eight supernova remnants...
We report on a 95 GHz (\({8}_{0}-{7}_{1}\) A+) methanol (CH3OH) emission survey with the Purple Mountain Observatory Delingha 13.7 m telescope. Eight supernova...
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SubjectTerms Emission
Galaxy: center
ISM: clouds
ISM: kinematics and dynamics
ISM: molecules
ISM: supernova remnants
Methanol
Molecular gases
Mountains
Polls & surveys
Star & galaxy formation
Star formation
Supernova
Supernova remnants
Title A 95 GHz methanol emission survey toward eight small supernova remnants
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