12CO (3-2) High-Resolution Survey (COHRS) of the Galactic Plane: Complete Data Release

被引：11

作者：

Park, Geumsook ^{[1
]}

Currie, Malcolm J. ^{[2
,3
]}

Thomas, Holly S. ^{[4
]}

Rosolowsky, Erik ^{[5
]}

Dempsey, Jessica T. ^{[2
,6
]}

Kim, Kee-Tae ^{[1
,7
]}

Rigby, Andrew J. ^{[8
,9
]}

Su, Yang ^{[10
,11
]}

Eden, David J. ^{[12
,13
]}

Colombo, Dario

Parsons, Harriet ^{[2
]}

Moore, Toby J. T. ^{[12
]}

机构：

[1] Korea Astron & Space Sci Inst, 776 Daedeokdae Ro, Daejeon 34055, South Korea

[2] East Asian Observ, 660 N Aohoku Pl, Hilo, HI 96720 USA

[3] RAL Space, STFC Rutherford Appleton Lab, Didcot OX11 0QX, Oxfordshire, England

[4] Radio Telescope Data Ctr, Ctr Astrophys Harvard & Smithsonian, 60 Garden St, Cambridge, MA 02138 USA

[5] Univ Alberta, Dept Phys, 4-181 CCIS, Edmonton, AB T6G 2E1, Canada

[6] ASTRON, Oude Hoogeveensedijk 4, NL-7991 PD Dwingeloo, Netherlands

[7] Univ Sci & Technol, Korea UST, 217 Gajeong Ro, Daejeon 34113, South Korea

[8] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, Wales

[9] Univ Leeds, Sch Phys & Astron, Leeds LS2 9JT, England

[10] Chinese Acad Sci, Purple Mt Observ, Hugel 69, Nanjing 210034, Peoples R China

[11] Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210034, Peoples R China

[12] Liverpool John Moores Univ, Astrophys Res Inst, IC2, Liverpool Sci Pk, 146 Brownlow Hill, Liverpool L3 5RF, Lancashire, England

[13] Armagh Observ & Planetarium, Coll Hill, Armagh BT61 9DG, North Ireland

来源：

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2023年 / 264卷 / 01期

基金：

新加坡国家研究基金会; 国家重点研发计划; 英国科学技术设施理事会; 加拿大自然科学与工程研究理事会;

关键词：

MULTIBEAM MASER CATALOG; MOLECULAR CLOUD; MILKY-WAY; STAR-FORMATION; CO SURVEY; EMISSION; RING; GAS; PARALLAXES; REDUCTION;

D O I：

10.3847/1538-4365/ac9b59

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the full data release of the (CO)-C-12 (3-2) High-Resolution Survey (COHRS), which has mapped the inner Galactic plane over the range of 9.& DEG;5 <= l 62.<= 3 and divide b divide & LE; 0.& DEG;5. COHRS has been carried out using the Heterodyne Array Receiver Program on the 15 m James Clerk Maxwell Telescope in Hawaii. The released data are smoothed to have a spatial resolution of 16.& DPRIME;6 and a velocity resolution of 0.635 km s(-1), achieving a mean rms of & SIM;0.6 K on TA* 12CO (1-0) and (3-2) and those of star-forming populations.

引用

页数：22

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