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相关论文: A Mapping Survey of Dense Clumps Associated with E…

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We have carried out a survey of the dense clumps associated with 14 embedded clusters in the C^18O (J=1-0) line emission with the Nobeyama 45m telescope in order to understand the formation and evolution of stellar clusters in dense clumps…

星系天体物理 · 物理学 2014-11-20 Aya E. Higuchi , Yasutaka Kurono , Masao Saito , Ryohei Kawabe

We report results of the observations of 15 regions in several molecular lines for a statistical study of massive cluster-forming clumps. We identified 24 clumps based on the C18O (J=1-0) data obtained by the NRO 45 m telescope, and found…

星系天体物理 · 物理学 2018-03-21 Tomomi Shimoikura , Kazuhito Dobashi , Fumitaka Nakamura , Tomoaki Matsumoto , Tomoya Hirota

Massive stars play an important role in the Universe. Unlike low-mass stars, the formation of these objects located at great distances is still unclear. It is expected to be governed by some combination of self-gravity, turbulence, and…

星系天体物理 · 物理学 2024-12-30 A. G. Pazukhin , I. I. Zinchenko , E. A. Trofimova

We present the results of C18O observations by the Nobeyama Millimeter Array toward dense clumps with radii of ~ 0.3 pc in six cluster-forming regions including massive (proto)stars. We identified 171 cores, whose radius, line width, and…

天体物理学 · 物理学 2009-11-13 Hiro Saito , Masao Saito , Yoshinori Yonekura , Fumitaka Nakamura

We report the statistical physical properties of the C$^{18}$O($J=1-0$) clumps present in a prominent cluster-forming region, Cygnus X, using the dataset obtained by the Nobeyama 45-m radio telescope. This survey covers 9 deg$^2$ of the…

Massive stars play an important role in the Universe. Unlike low-mass stars, the formation of these objects located at great distances is still unclear. It is expected to be governed by some combination of self-gravity, turbulence, and…

星系天体物理 · 物理学 2024-08-07 A. G. Pazukhin , I. I. Zinchenko , E. A. Trofimova

We have carried out a survey of the NGC 2068 region in the Orion B molecular cloud using HARP on the JCMT, in the 13CO and C18O (J = 3-2) and H13CO+ (J = 4-3) lines. We used 13CO to map the outflows in the region, and matched them with…

星系天体物理 · 物理学 2015-06-12 S. L. Walker-Smith , J. S. Richer , J. V. Buckle , R. J. Smith , J. S. Greaves , I. A. Bonnell

We present FCRAO maps as well as combined BIMA and FCRAO maps of the high density molecular emission towards the CS core in the L673 region. With the FCRAO telescope, we mapped the emission in the CS(2-1), C34S(2-1), HCO+(1-0), and…

天体物理学 · 物理学 2009-11-10 Oscar Morata , Josep Miquel Girart , Robert Estalella

We have used the IRAM 30-m telescope to map some targets with HCO$^+$ (1-0) and H$^{13}$CO$^+$ (1-0) lines in order to search for gas infall evidence in the clumps. In this paper, we report the mapping results for 13 targets. All of these…

星系天体物理 · 物理学 2023-08-03 Yang Yang , Xi Chen , Zhibo Jiang , Zhiwei Chen , Shuling Yu , Jun Li

We present observations of HCO+ and H^13CO+, N2H+, HCS+, HCN and HN^13C, SO and ^34SO, CCH, SO_2, and CH_3OH-E towards a sample of 27 high-mass clumps coincident with water maser emission. All transitions are observed with or convolved to…

星系天体物理 · 物理学 2015-05-27 Megan Reiter , Yancy Shirley , Jingwen Wu , Crystal Brogan , Alwyn Wootten , Ken'ichi Tatematsu

We present high resolution observations of CS(J=1-0), H13CO+ (J=1-0), and SiO(v=0:J=1-0) lines, together with the 49GHz and 86GHz continuum emissions, toward W49N carried out with Nobeyama Millimeter Array. We identified 11 CS, 8 H13CO+,…

星系天体物理 · 物理学 2021-12-15 Ryosuke Miyawaki , Masahiko Hayashi , Tetsuo Hasegawa

A survey toward 674 Planck cold clumps of the Early Cold Core Catalogue (ECC) in the J=1-0 transitions of $^{12}$CO, $^{13}$CO and C$^{18}$O has been carried out using the PMO 13.7 m telescope. 673 clumps were detected with the $^{12}$CO…

太阳与恒星天体物理 · 物理学 2015-06-05 Yuefang Wu , Tie Liu , Fanyi Meng , Di Li , Sheng-Li Qin , Bing-Gang Ju

We present maps of 7 young massive molecular clumps within 5 target regions in the C18O (J=1-0) line emission, using the Nobeyama 45m telescope. These clumps, which are not associated with clusters, lie at distances between 0.7 to 2.1 kpc.…

星系天体物理 · 物理学 2015-06-12 Aya E. Higuchi , Yasutaka Kurono , Takahiro Naoi , Masao Saito , Rainer Mauersberger , Ryohei Kawabe

We have mapped over 50 massive, dense clumps with four dense gas tracers: HCN J=1-0 and 3-2; and CS J=2-1 and 7-6 transitions. Spectral lines of optically thin H^{13}CN 3-2 and C^{34}S 5-4 were also obtained towards the map centers. These…

星系天体物理 · 物理学 2015-05-18 Jingwen Wu , Neal Evans , Yancy Shirley , Claudia Knez

We present $\sim$100 pc resolution Hubble Space Telescope H$\alpha$ images of 10 galaxies from the DYnamics of Newly-Assembled Massive Objects (DYNAMO) survey of low-$z$ turbulent disk galaxies, and use these to undertake the first detailed…

We report results of a project to map HCN and HCO+ J = 1-0 emission toward a sample of molecular clouds in the inner Galaxy, all containing dense clumps that are actively engaged in star formation. We compare these two molecular line…

星系天体物理 · 物理学 2020-05-20 Neal J. Evans , Kee-Tae Kim , Jingwen Wu , Zhang Chao , Mark Heyer , Tie Liu , Quang Nguyen-Luong , Jens Kauffmann

Infrared-dark high-mass clumps are among the most promising objects to study the initial conditions of the formation process of high-mass stars and rich stellar clusters. In this work, we have observed the (3-2) rotational transition of…

星系天体物理 · 物理学 2015-06-04 F. Fontani , A. Giannetti , M. T. Beltran , R. Dodson , M. Rioja , J. Brand , P. Caselli , R. Cesaroni

We report new near-infrared and mm-wave observational data on a selection of massive Galactic molecular clumps (part of the CHaMP sample) and their associated young star clusters. The clumps show, for the first time in a "dense gas tracer",…

We investigate the infall properties in a sample of 11 infrared dark clouds (IRDCs) showing blue-asymmetry signatures in HCO$^{+}$ J=1--0 line profiles. We used JCMT to conduct mapping observations in HCO$^{+}$ J=4--3 as well as…

Some well-studied Herbig Haro objects have associated with them one or more cold, dense, and quiescent clumps of gas. We propose that such clumps near an HH object can be used as a general measure of clumpiness in the molecular cloud that…

星系天体物理 · 物理学 2015-05-14 W. Whyatt , J. M. Girart , S. Viti , R. Estalella , D. A. Williams
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