中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Accurate OH Maser Positions from the SPLASH Survey. III. The Final 96 deg(2)

文献类型:期刊论文

作者Qiao, Hai-Hua10,11; Breen, Shari L.7,8,9; Gomez, Jose F.6; Dawson, J. R.7,8; Walsh, Andrew J.7,8; Green, James A.5; Ellingsen, Simon P.4; Imai, Hiroshi2,3; Shen, Zhi-Qiang1,10
刊名ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
出版日期2020-03-01
卷号247期号:1页码:22
ISSN号0067-0049
DOI10.3847/1538-4365/ab655d
英文摘要We present high spatial resolution observations of ground-state OH masers achieved with the Australia Telescope Compact Array (ATCA). These observations targeted 253 pointing centers containing OH maser candidates at all four ground-state OH transitions identified in the Southern Parkes Large-Area Survey in Hydroxyl (SPLASH) across 96 deg(2) of the southern Galactic plane (332 degrees < l < 334 degrees and -2 degrees < b <+2 degrees, 344 degrees < l < 355 degrees and -2 degrees < b< +2 degrees, 358 degrees < l < 4 degrees and +2 degrees < b<+6 degrees, 5 degrees < l < 10 degrees and -2 degrees < b <+2 degrees). We detect maser emission toward 236 fields and suggest that 7 out of 17 nondetections are due to the slightly lower sensitivity of the ATCA observations, combined with some temporal variability. The superior resolution provided by the ATCA data has allowed us to identify 362 OH maser sites in the 236 target fields. Almost half (160 of 362) of these masers have been detected for the first time. Comparison between these 362 maser sites and information presented in the literature allowed us to categorize 238 sites as evolved star sites (66%), 63 as star formation (17%), 8 as supernova remnants, and 53 as unknown maser sites (15%). We present an analysis of the OH masers across the full SPLASH survey range (176 deg(2)) and find that the detection rate of 1.7 GHz radio continuum sources (18%) is lower than that previously found at 8.2 and 9.2 GHz (38%). We also find that the velocity separations of evolved star sites with symmetric 1612 MHz maser profiles are generally smaller than those with asymmetric profiles.
WOS关键词POST-AGB STARS ; FULL POLARIZATION SPECTRA ; ASYMPTOTIC-GIANT-BRANCH ; YOUNG PLANETARY-NEBULA ; 1612 MHZ SURVEY ; METHANOL MASERS ; IRAS SOURCES ; SUPERNOVA-REMNANTS ; HYDROXYL MASERS ; VARIABLE-STARS
资助项目Commonwealth of Australia ; NASA ; Center for Astronomical Mega-Science, Chinese Academy of Sciences (CAMS-CAS) ; CAS "Light of West China" Program ; National Natural Science Foundation of China[11903038] ; MINECO (Spain)[AYA2017-84390-C2-1-R] ; FEDER ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award[SEV-20170709] ; Major Program of the National Natural Science Foundation of China[11590780] ; Major Program of the National Natural Science Foundation of China[11590784] ; CAS Pioneer Hundred Talents Program[Y650YC1201] ; JSPS[25610043] ; JSPS[16H02167]
WOS研究方向Astronomy & Astrophysics
语种英语
出版者IOP PUBLISHING LTD
WOS记录号WOS:000537501600005
资助机构Commonwealth of Australia ; Commonwealth of Australia ; NASA ; NASA ; Center for Astronomical Mega-Science, Chinese Academy of Sciences (CAMS-CAS) ; Center for Astronomical Mega-Science, Chinese Academy of Sciences (CAMS-CAS) ; CAS "Light of West China" Program ; CAS "Light of West China" Program ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; MINECO (Spain) ; MINECO (Spain) ; FEDER ; FEDER ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award ; Major Program of the National Natural Science Foundation of China ; Major Program of the National Natural Science Foundation of China ; CAS Pioneer Hundred Talents Program ; CAS Pioneer Hundred Talents Program ; JSPS ; JSPS ; Commonwealth of Australia ; Commonwealth of Australia ; NASA ; NASA ; Center for Astronomical Mega-Science, Chinese Academy of Sciences (CAMS-CAS) ; Center for Astronomical Mega-Science, Chinese Academy of Sciences (CAMS-CAS) ; CAS "Light of West China" Program ; CAS "Light of West China" Program ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; MINECO (Spain) ; MINECO (Spain) ; FEDER ; FEDER ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award ; Major Program of the National Natural Science Foundation of China ; Major Program of the National Natural Science Foundation of China ; CAS Pioneer Hundred Talents Program ; CAS Pioneer Hundred Talents Program ; JSPS ; JSPS ; Commonwealth of Australia ; Commonwealth of Australia ; NASA ; NASA ; Center for Astronomical Mega-Science, Chinese Academy of Sciences (CAMS-CAS) ; Center for Astronomical Mega-Science, Chinese Academy of Sciences (CAMS-CAS) ; CAS "Light of West China" Program ; CAS "Light of West China" Program ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; MINECO (Spain) ; MINECO (Spain) ; FEDER ; FEDER ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award ; Major Program of the National Natural Science Foundation of China ; Major Program of the National Natural Science Foundation of China ; CAS Pioneer Hundred Talents Program ; CAS Pioneer Hundred Talents Program ; JSPS ; JSPS ; Commonwealth of Australia ; Commonwealth of Australia ; NASA ; NASA ; Center for Astronomical Mega-Science, Chinese Academy of Sciences (CAMS-CAS) ; Center for Astronomical Mega-Science, Chinese Academy of Sciences (CAMS-CAS) ; CAS "Light of West China" Program ; CAS "Light of West China" Program ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; MINECO (Spain) ; MINECO (Spain) ; FEDER ; FEDER ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award ; Major Program of the National Natural Science Foundation of China ; Major Program of the National Natural Science Foundation of China ; CAS Pioneer Hundred Talents Program ; CAS Pioneer Hundred Talents Program ; JSPS ; JSPS
源URL[http://210.72.145.45/handle/361003/9358]  
专题国家授时中心_守时理论与方法研究室
通讯作者Qiao, Hai-Hua
作者单位1.Chinese Acad Sci, Key Lab Radio Astron, Shanghai, Peoples R China
2.Kagoshima Univ, Grad Sch Sci & Engn, Dept Phys & Astron, 1-21-35 Korimoto, Kagoshima 8900065, Japan
3.Kagoshima Univ, Ctr Gen Educ, 1-21-30 Korimoto, Kagoshima 8900065, Japan
4.Univ Tasmania, Sch Phys Sci, Private Bag 37, Hobart, Tas 7001, Australia
5.CSIRO Astron & Space Sci, Australia Telescope Natl Facil, POB 76, Epping, NSW 2121, Australia
6.CSIC, Inst Astrofis Andalucia, Glorieta Astron S-N, E-18008 Granada, Spain
7.Macquarie Univ, MQ Res Ctr Astron, N Ryde, NSW 2109, Australia
8.Macquarie Univ, Dept Phys & Astron, N Ryde, NSW 2109, Australia
9.Univ Sydney, Sydney Inst Astron SIfA, Sch Phys, Sydney, NSW 2006, Australia
10.Chinese Acad Sci, Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China
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Qiao, Hai-Hua,Breen, Shari L.,Gomez, Jose F.,et al. Accurate OH Maser Positions from the SPLASH Survey. III. The Final 96 deg(2)[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,2020,247(1):22.
APA Qiao, Hai-Hua.,Breen, Shari L..,Gomez, Jose F..,Dawson, J. R..,Walsh, Andrew J..,...&Shen, Zhi-Qiang.(2020).Accurate OH Maser Positions from the SPLASH Survey. III. The Final 96 deg(2).ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,247(1),22.
MLA Qiao, Hai-Hua,et al."Accurate OH Maser Positions from the SPLASH Survey. III. The Final 96 deg(2)".ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 247.1(2020):22.

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