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researcher

T. Henning

48 papers hereh-index 10360 citations55 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author41
  • last author1

Across the 42 of 48 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA24
  • astro-ph.SR15
  • astro-ph.EP7
  • astro-ph1
  • astro-ph.HE1
same name
  • T. Henning — 699 papers, h 104
  • T. Henning — 177 papers, h 43
  • T. Henning — 95 papers, h 41
  • T. Henning — 83 papers, h 34
  • T. Henning — 74 papers, h 22
  • T. Henning — 62 papers, h 15

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20082026
most citedThe earliest phases of star formation - A Herschel key project. The thermal structure of low-mass molecular cloud cores

169 citations · 1.1k across the 45 of their papers we have counts for

collaborators
Showing 2010Show all

3 papers · 1 filter

astro-ph.GA2010★ 49 cited

First detection of ND in the solar-mass protostar IRAS16293-2422

A. Bacmann, E. Caux, P. Hily-Blant +64

In the past decade, much progress has been made in characterising the processes leading to the enhanced deuterium fractionation observed in the ISM and in particular in the cold, d…

astro-ph.GA2010★ 115 cited

The CHESS chemical Herschel surveys of star forming regions: Peering into the protostellar shock L1157-B1. I. Shock chemical complexity

C. Codella, B. Lefloch, C. Ceccarelli +2

We present the first results of the unbiased survey of the L1157-B1 bow shock, obtained with HIFI in the framework of the key program Chemical Herschel surveys of star forming regi…

astro-ph.GA2010★ 54 cited

Sequential Star Formation in RCW 34: A Spectroscopic Census of the Stellar Content of High-mass Star-forming Regions

A. Bik, E. Puga, L. B. F. M. Waters +16

We present VLT/SINFONI integral field spectroscopy of RCW 34 along with Spitzer/IRAC photometry of the surroundings. RCW 34 consists of three different regions. A large bubble has…

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