Zhiyuan Ren - NAOC, PKU

Zhiyuan Ren
Are you Zhiyuan Ren?

Claim your profile, edit publications, add additional information:

Contact Details

Name
Zhiyuan Ren
Affiliation
NAOC, PKU
Location

Pubs By Year

Pub Categories

 
Solar and Stellar Astrophysics (7)
 
Astrophysics of Galaxies (5)

Publications Authored By Zhiyuan Ren

Stellar feedback from high-mass stars can strongly influence the surrounding interstellar medium and regulate star formation. Our new ALMA observations reveal sequential high-mass star formation taking place within one sub-virial filamentary clump (the G9.62 clump) in the G9. Read More

We present a Submillimeter Array (SMA) observation towards the young massive double-core system G350.69-0.49. Read More

We present a multi-wavelength observational study of the NGC 2024 filament using infrared to sub-millimeter continuum and the NH$_3$ $(1,1)$ and $(2,2)$ inversion transitions centered on FIR-3, the most massive core therein. FIR-3 is found to have no significant infrared point sources in the Spitzer/IRAC bands. But the NH$_3$ kinetic temperature map shows a peak value at the core center with $T_{\rm k}=25$ K which is significantly higher than the surrounding level ($T_{\rm k}=15-19$ K). Read More

2014Apr

Context: We investigated the molecular gas associated with 6.7 GHz methanol masers throughout the Galaxy using a J=1-0 transition of the CO isotopologues. Methods:Using the 13. Read More

We present a high-resolution $1.5"$ observational study towards two massive dust-and-gas cores, ORI8nw\_2 and ORI2\_6 in Orion Molecular Cloud using the Combined Array for Research in Millimeter-wave Astronomy (CARMA). In both regions the 3. Read More

We present the results of a high resolution study with the Submillimeter Array towards the massive star forming complex G9.62+0.19. Read More

We present a high-resolution study of a massive dense core JCMT 18354-0649S with the Submillimeter Array. The core is mapped with continuum emission at 1.3 mm, and molecular lines including CH$_{3}$OH ($5_{23}$-$4_{13}$) and HCN (3-2). Read More