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
Showing astro-ph.GAShow all

10 papers · 1 filter

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…

astro-ph.GA2021★ 8 cited

Observations of multiple NH transitions in W33

K. Tursun, C. Henkel, J. Esimbek +10

At a distance of 2.4kpc, W33 is an outstanding massive and luminous 10pc sized star forming complex containing quiescent infrared dark clouds as well as highly active infrared brig…

astro-ph.GA2020★ 22 cited

Galactic interstellar sulfur isotopes: A radial SS gradient?

H. Z. Yu, J. S. Zhang, C. Henkel +9

We present observations of CS, CS, CS and CS J=21 lines toward a large sample of massive star forming regions by using th…

astro-ph.GA2019★ 67 cited

A systematic TMRT observational study of Galactic C/C ratios from Formaldehyde

Y. T. Yan, J. S. Zhang, C. Henkel +10

We present observations of the C-band (4.8 GHz) and Ku-band (14.5 GHz) K-doublet lines of HCO and the C-band (4.6 GHz) line of H…

astro-ph.GA2017★ 36 cited

Kinetic temperature of massive star-forming molecular clumps measured with formaldehyde. III. The Orion Molecular Cloud 1

X. D. Tang, C. Henkel, K. M. Menten +10

We mapped the kinetic temperature structure of the Orion molecular cloud 1 with para-H2CO(303-202, 322-221, and 321-220) using the APEX 12m telescope. This is compared with the tem…

astro-ph.GA2016★ 39 cited

Kinetic temperature of massive star forming molecular clumps measured with formaldehyde

X. D. Tang, C. Henkel, K. M. Menten +8

For a general understanding of the physics involved in the star formation process, measurements of physical parameters such as temperature and density are indispensable. The chemic…