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researcher

D. Semenov

33 papers hereh-index 8312 citations42 works total

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

author position
  • first author1
  • middle author25
  • last author3

Across the 29 of 33 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA18
  • astro-ph.SR9
  • astro-ph.EP6
same name
  • D. Semenov — 75 papers, h 32
  • D. Semenov — 51 papers, h 36
  • D. Semenov — 10 papers, h 3
  • D. Semenov — 10 papers, h 6
  • D. Semenov — 7 papers, h 5
  • D. Semenov — 6 papers, h 2

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
20162026
most citedPRODIGE -- Envelope to disk with NOEMA I. A 3000 au streamer feeding a Class I protostar

100 citations · 365 across the 26 of their papers we have counts for

collaborators
Showing 2026 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2026

The Cygnus Allscale Survey of Chemistry and Dynamical Environments: CASCADE: VI. Molecular outflows in the DR21 ridge

I. M. Skretas, A. Karska, F. Wyrowski +8

Star formation takes place in varied environments, from isolated clumps to massive molecular cloud complexes. However, whether the environment in which a star forms has any effect…

astro-ph.GA2026★ 1 cited

PRODIGE - envelope to disk with NOEMA: VII. (Complex) organic molecules in the NGC1333 IRAS4B1 outflow: A new laboratory for shock chemistry

Laura A. Busch, J. E. Pineda, P. Caselli +20

Shock chemistry is an excellent tool to shed light on the formation and destruction mechanisms of complex organic molecules (COMs). The L1157-mm outflow is the only low-mass protos…

astro-ph.GA2026

The converging gas flow around the infrared dark cloud G28.3

H. Beuther, C. Gieser, H. Linz +7

Aims: The G28.37+0.07 star-forming region is a prototypical infrared dark cloud (IRDC) located at the interface of a converging gas flow. This study characterizes the properties of…

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