activity
20102026
most citedThe ALMA Survey of 70 m dark High-mass clumps in Early Stages (ASHES). I. Pilot Survey: Clump Fragmentation

207 citations · 4.3k across the 150 of their papers we have counts for

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40 papers · 1 filter

astro-ph.SR2022★ 6 cited

Formation and Eruption of Hot Channels during an M6.5 Class Solar Flare

Yanjie Liu, Yingna Su, Rui Liu +3

We investigate the formation and eruption of hot channels associated with the M6.5 class flare (SOL2015-06-22T18:23) occurring in NOAA AR 12371 on 2015 June 22. Two flare precursor…

astro-ph.SR2021★ 22 cited

Partial Eruption, Confinement, and Twist Buildup and Release of a Double-decker Filament

Jialin Chen, Yingna Su, Rui Liu +4

We investigate the failed partial eruption of a filament system in NOAA AR 12104 on 2014 July 5, using multiwavelength EUV, magnetogram, and H observations, as well as magnetic…

astro-ph.SR2021★ 2 cited

The JCMT Transient Survey: Four Year Summary of Monitoring the Submillimeter Variability of Protostars

Yong-Hee Lee, Doug Johnstone, Jeong-Eun Lee +49

We present the four-year survey results of monthly submillimeter monitoring of eight nearby (pc) star-forming regions by the JCMT Transient Survey. We apply the Lomb-Scargl…

astro-ph.SR2021★ 15 cited

Tether-cutting and Overlying Magnetic Reconnections in an MHD Simulation of Prominence-cavity System

Tie Liu, Yingna Su

We investigate the magnetic reconnection in an MHD simulation of a coronal magnetic flux rope (MFR) confined by a helmet streamer, where a prominence-cavity system forms. This syst…

astro-ph.SR2020★ 11 cited

G133.50+9.01: A likely cloud-cloud collision complex triggering the formation of filaments, cores and a stellar cluster

Namitha Issac, Anandmayee Tej, Tie Liu +1

We present compelling observational evidence of G133.50+9.01 being a bona fide cloud-cloud collision candidate with signatures of induced filament, core, and cluster formation. The…

astro-ph.SR2020★ 10 cited

Multiwavelength investigation of extended green object G19.88-0.53: Revealing a protocluster

Namitha Issac, Anandmayee Tej, Tie Liu +5

A multiwavelength analysis of star formation associated with the extended green object, G19.88-0.53 is presented in this paper. With multiple detected radio and millimetre componen…

astro-ph.SR2020★ 28 cited

ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): I. Detection of New Hot Corinos with ACA

Shih-Ying Hsu, Sheng-Yuan Liu, Tie Liu +29

We report the detection of four new hot corino sources, G211.47-19.27S, G208.68-19.20N1, G210.49-19.79W and G192.12-11.10 from a survey study of Planck Galactic Cold Clumps in the…

astro-ph.SR2019★ 4 cited

Formation and Eruption of a Mini-sigmoid Originating in Coronal Hole

Z. W. Huang, X. Cheng, Y. N. Su +2

In this paper, we study in detail the evolution of a mini-sigmiod originating in a cross-equatorial coronal hole, where the magnetic field is mostly open and seriously distinct fro…

astro-ph.SR2019★ 7 cited

The Nearby Evolved Stars Survey: I. JCMT/SCUBA-2 Sub-millimetre detection of the detached shell of U Antliae

Thavisha E. Dharmawardena, Francisca Kemper, Sundar Srinivasan +24

We present the highest resolution single-dish submillimetre observations of the detached shell source U Antliae to date. The observations were obtained at $450~\micron$ and $850~\m…

astro-ph.SR2019★ 4 cited

Sequential Star Formation in the filamentary structures of Planck Galactic cold clump G181.84+0.31

Lixia Yuan, Ming Zhu, Tie Liu +7

We present a multi-wavelength study of the Planck cold clump G181.84+0.31, which is located at the northern end of the extended filamentary structure S242. We have extracted 9 comp…

astro-ph.SR2019★ 14 cited

Carbon-Chain Molecules in Molecular Outflows and Lupus I Region--New Producing Region and New Forming Mechanism

Yuefang Wu, Xunchuan Liu, Xi Chen +18

Using the new equipment of the Shanghai Tian Ma Radio Telescope, we have searched for carbon-chain molecules (CCMs) towards five outflow sources and six Lupus I starless dust cores…

astro-ph.SR2019★ 10 cited

A particular carbon-chain-producing region: L1489 starless core

Yuefang Wu, Lianghao Lin, Xunchuan Liu +14

We detected carbon-chain molecules (CCMs) HC2n+1N (n=1-3) and C3S in Ku band as well as {high-energy excitation lines including C4H N=9-8, J=17/2-15/2, 19/2-17/2, and CH3CCH J=5-4,…

astro-ph.SR2019★ 25 cited

MHD simulation of prominence-cavity system

Yuhong Fan, Tie Liu

We present magnetohydrodynamic simulation of the evolution from quasi-equilibrium to onset of eruption of a twisted, prominence-forming coronal magnetic flux rope underlying a coro…

astro-ph.SR2019★ 17 cited

C2H N=1-0 and N2H+ J=1-0 observations of Planck Galactic cold clumps

Xunchuan Liu, Yuefang Wu, Chao Zhang +5

A survey of C2H N=1-0 and N2H+ J=1-0 toward Planck Galactic cold clumps (PGCCs) was performed using the Purple Mountain Observatory's 13.7 m telescope. C2H and N2H+ were chosen to…

astro-ph.SR2018★ 11 cited

Compressed magnetic field in the magnetically-regulated global collapsing clump of G9.62+0.19

Tie Liu, Kee-Tae Kim, Sheng-Yuan Liu +22

How stellar feedback from high-mass stars (e.g., H{\sc ii} regions) influences the surrounding interstellar medium and regulates new star formation is still unclear. To address thi…

astro-ph.SR2018★ 21 cited

Magnetic Field Modeling of hot channels in Four Flare/CME Events

Tie Liu, Yingna Su, Xin Cheng +2

We investigate the formation and magnetic topology of four flare/CME events with filament-sigmoid systems, in which the sigmoidal hot channels are located above the filaments, and…

astro-ph.SR2018

First detection of vibrationally excited Glycolaldehyde in the solar-type protostar IRAS 16293-2422

Yan Zhou, Sheng-Li Qin, Alvaro Sanchez-Monge +7

This paper was withdrawed from the ApJ after the comments from the referee, please be carefully.

astro-ph.SR2015★ 27 cited

SMA observations of the W3(OH) complex: Dynamical differentiation between W3(HO) and W3(OH)

Sheng-Li Qin, Peter Schilke, Jingwen Wu +4

We present Submillimeter Array (SMA) observations of the HCN\,(3--2) and HCO\,(3--2) molecular lines toward the W3(HO) and W3(OH) star-forming complexes. Infall and outflow…

astro-ph.SR2015★ 1 cited

High-resolution CO observation of the carbon star CIT 6 revealing the spiral structure and a nascent bipolar outflow

Hyosun Kim, Sheng-Yuan Liu, Naomi Hirano +8

CIT 6 is a carbon star in the transitional phase from the asymptotic giant branch (AGB) to the protoplanetary nebulae (pPN). Observational evidences of two point sources in the opt…

astro-ph.SR2015★ 9 cited

Extremely Energetic Outflow and Decelerated Expansion in W49N

Tie Liu, Kee-Tae Kim, Yuefang Wu +10

W49N is a mini-starburst in the Milky Way and thus an ideal laboratory for high-mass star formation studies. Due to its large distance (11.1 kpc), the kinematics in…

astro-ph.SR2015★ 32 cited

SMA Observations of W3(OH) Complex: Physical and Chemical Differentiation between W3(HO) and W3(OH)

Sheng-Li Qin, Peter Schilke, Jingwen Wu +4

We report on the Submillimeter Array (SMA) observations of molecular lines at 270 GHz toward W3(OH) and W3(HO) complex. Although previous observations already resolved the W3(H…

astro-ph.SR2014★ 44 cited

A feedback-driven bubble G24.136+00.436: a possible site of triggered star formation

Hong-Li Liu, Yuefang Wu, JinZeng Li +3

We present a multi-wavelength study of the IR bubble G24.136+00.436. The J=1-0 observations of CO, CO and CO were carried out with the Purple Mountain Observat…

astro-ph.SR2014

Inflows in massive star formation regions

Yuefang Wu, Tie Liu, Shengli Qin

How high-mass stars form remains unclear currently. Calculation suggests that the radiation pressure of a forming star can halt spherical infall, preventing its further growth when…

astro-ph.SR2014

Follow-up observations toward Planck cold clumps with ground-based radio telescopes

Tie Liu, Yuefang Wu, Diego Mardones +26

The physical and chemical properties of prestellar cores, especially massive ones, are still far from being well understood due to the lack of a large sample. The low dust temperat…