supported by the National Key R&D Program of China(Grant No.2017YFA0402702);the National Natural Science Foundation of China(NSFC,Grant Nos.,11873093,U2031202,and 11903083);sponsored by the National Key R&D Program of China with Grant 2017YFA0402701;CAS Key Research Program of Frontier Sciences with grant QYZDJ-SSW-SLH047。
We have started a systematic survey of molecular clumps with infall motions to study the very early phase of star formation.Our first step is to utilize the data products by MWISP to make an unbiased survey for blue a...
supported by the National Key R&D Program of China (Grant No. 2017YFA0402702);National Natural Science Foundation of China (NSFC, Grant Nos.11873093 and U2031202);support from the NSFC (Grant No. 11903083)。
The research of infall motion is a common means to study molecular cloud dynamics and the early process of star formation. Many works had been done in-depth research on infall. We searched the literature related to in...
In the paper“In Search for Infall Motion in molecular clumps II:HCO+(1-0)and HCN(1-0)Observations toward a Sub-sample of Infall Candidates”by Yang etal.(RAA 2020 Vol.20 No.8,115(14pp),doi:10.1088/1674C4527/20/8/115)...
supported by the National Natural Science Foundation of China (NSFC,Grant Nos.11988101,11725313,and 11721303);the International Partnership Program of Chinese Academy of Sciences (Grant No.114A11KYSB20160008);the National Key R&D Program of China (No.2016YFA0400702)。
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 a...
the National Key Reasearch and Development Program of China(Nos.2017YFA0402701 and 2019YFA0405100);the National Natural Science Foundation of China(U1631237,11973013,11721303,11373026 and 11433004);the starting grant at the Kavli Institute for Astronomy and Astrophysics,Peking University(7101502016)。
Thirty massive clumps associated with bright infrared sources were observed to detect the infall signatures and characterize infall properties in the envelope of the massive clumps by APEX telescope in CO(4-3)and C17O...
the National Key R&D Program of China(Grant No.2017YFA0402702);the National Natural Science Foundation of China(NSFC,Grant Nos.10873037,11873093,11803091 and 11933011);the National Key R&D Program of China(Grant No.2017YFA0402700);the Key Research Program of Frontier Sciences,CAS(Grant No.QYZDJ-SSWSLH047)。
Gravitational accretion accumulates the original mass.This process is crucial for us to understand the initial phases of star formation.Using the specific infall profiles in optically thick and thin lines,we searched ...
supportedby the National Key R&D Program of China (No.2017YFA0402701);by the National Natural Science Foundation of China (Grant Nos. 11373026 and11433004);the Joint Research Fund in Astronomy(U1631237) under cooperative agreement between the National Natural Science Foundation of China and Chinese Academy of Sciences;by the Top TalentsProgram of Yunnan Province (2015HA030);by Yunnan University’s Research Innovation Fund for Graduate Students
Previous observations have revealed an accretion disk and outflow motion in the high-mass starforming region G192.16–3.84, but collapse has not been reported before. Here we present molecular line and continuum obser...
This work was performed under the auspices of Max-Planck Society of Germany;the National NaturaI Science Foundation of China
Unusual activity of outflow mass motion connected with infall events was recorded for the B0.5 IVe star FY CMa in February 1987 from both archival IUE spectrograms of circumstellar N v resonance lines and optical spec...
The cluster-galaxy cross-correlation and the average infall velocity around cluster for the tilted CDM models, the hot-cold mixed dark matter models (MDM) and theA CDM models are calculated. And it is found that the p...