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researcher

J. Stutzki

94 papers hereh-index 438.3k citations340 works total

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

author position
  • first author1
  • middle author66
  • last author18

Across the 85 of 94 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA60
  • astro-ph13
  • astro-ph.IM8
  • astro-ph.CO4
  • astro-ph.SR4
  • astro-ph.EP3
same name
  • J. Stutzki — 38 papers, h 13
  • J. Stutzki — 26 papers, h 29
  • J. Stutzki — 4 papers, h 9
  • J. Stutzki — 3 papers, h 7

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
19962024
most citedThe Cologne Database for Molecular Spectroscopy, CDMS, in the Virtual Atomic and Molecular Data Centre, VAMDC

803 citations · 5.5k across the 94 of their papers we have counts for

collaborators
Showing 2009Show all

3 papers · 1 filter

astro-ph.CO2009★ 40 cited

Warm and Dense Molecular Gas in the N159 Region: 12CO J=4-3 and 13CO J=3-2 Observations with NANTEN2 and ASTE

Yoji Mizuno, Akiko Kawamura, Toshikazu Onishi +29

New 12CO J=4-3 and 13CO J=3-2 observations of the N159 region in the Large Magellanic Cloud have been made. The 12CO J=4-3 distribution is separated into three clumps. These new me…

astro-ph.GA2009★ 22 cited

Temperature and Density in the Foot Points of the Molecular Loops in the Galactic Center; Analysis of Multi-J Transitions of 12CO(J=1-0, 3-2, 4-3, 7-6), 13CO(J=1-0) and C18O(J=1-0)

Kazufumi Torii, Natsuko Kudo, Motosuji Fujishita +22

Fukui et al. (2006) discovered two molecular loops in the Galactic center and argued that the foot points of the molecular loops, two bright spots at both loops ends, represent the…

astro-ph.GA2009★ 16 cited

The molecular environment of the massive star forming region NGC 2024: Multi CO transition analysis

M. Emprechtinger, M. C. Wiedner, R. Simon +10

NGC 2024, a sites of massive star formation, have complex internal structures caused by cal heating by young stars, outflows, and stellar winds. These complex cloud structures lead…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.