activity
20022026
most citedA Shorter 146Sm Half-Life Measured and Implications for 146Sm-142Nd Chronology in the Solar System

183 citations · 676 across the 21 of their papers we have counts for

collaborators

21 papers

physics.ins-det2026

EBS and in-beam -ray investigation of FCVA-prepared CrO targets for low-energy O+O fusion experiments

C. Wen, X. Chen, L. Wang +22

The CrO solid target for low-energy O+O fusion experiments was fabricated using filtered cathodic vacuum arc (FCVA) deposition. Its composition, oxygen areal…

astro-ph.GA2026

Kinetic temperature of massive star-forming molecular clumps measured with formaldehyde VI. The photodissociation region M17SW

X. Zhao, X. D. Tang, C. Henkel +20

The kinetic temperature structure of the photodissociation region M17SW was mapped using the IRAM 30 m telescope. This mapping employed the para-H2CO triplet (J(KaKc) = 303-202, 32…

astro-ph.GA2026

Molecular Clouds at the Edge of the Galaxy II. Physical properties and scaling relations

C. S. Luo, X. D. Tang, C. Henkel +22

The outer Galaxy presents an optimal setting for investigating molecular clouds and star formation in environments with low metallicity. A total of 72 Galactic edge clouds were sur…

astro-ph.GA2024★ 9 cited

Kinetic temperature of massive star-forming molecular clumps measured with formaldehyde V. The massive filament DR21

X. Zhao, X. D. Tang, C. Henkel +18

The kinetic temperature structure of the massive filament DR21 has been mapped using the IRAM 30 m telescope. This mapping employed the para-HCO triplet ( = 3$_…

astro-ph.GA2023★ 6 cited

Protonated hydrogen cyanide as a tracer of pristine molecular gas

Y. Gong, F. J. Du, C. Henkel +11

Protonated hydrogen cyanide, HCNH, plays a fundamental role in astrochemistry because it is an intermediary in gas-phase ion-neutral reactions within cold molecular clouds. H…

astro-ph.GA2022★ 8 cited

Interstellar Nitrogen Isotope Ratios: New NH3 Data from the Galactic Center out to the Perseus Arm

J. L. Chen, J. S. Zhang, C. Henkel +10

Our aim is to measure the interstellar 14N/15N ratio across the Galaxy, to establish a standard data set on interstellar ammonia isotope ratios, and to provide new constraints on t…