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researcher

M. Griffin

4 papers here

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

author position
  • middle author4

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO3
  • astro-ph.GA1
same name
  • M. Griffin — 88 papers, h 45
  • M. Griffin — 54 papers, h 41
  • M. Griffin — 17 papers, h 12
  • M. Griffin — 6 papers, h 2
  • M. Griffin — 3 papers, h 4
  • M. Griffin — 3 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

most citedThe Herschel Space Observatory view of dust in M81

165 citations · 310 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2010★ 47 cited

Herschel observations of embedded protostellar clusters in the Rosette Molecular Cloud

M. Hennemann, F. Motte, S. Bontemps +39

The Herschel OB young stellar objects survey (HOBYS) has observed the Rosette molecular cloud, providing an unprecedented view of its star formation activity. These new far-infrare…

astro-ph.CO2010★ 37 cited

Mapping the interstellar medium in galaxies with Herschel/SPIRE

S. A. Eales, M. W. L. Smith, C. D. Wilson +57

The standard method of mapping the interstellar medium in a galaxy, by observing the molecular gas in the CO 1-0 line and the atomic gas in the 21-cm line, is largely limited with…

astro-ph.CO2010★ 165 cited

The Herschel Space Observatory view of dust in M81

G. J. Bendo, C. D. Wilson, M. Pohlen +57

We use Herschel Space Observatory data to place observational constraints on the peak and Rayleigh-Jeans slope of dust emission observed at 70-500 microns in the nearby spiral gala…

astro-ph.CO2010★ 61 cited

Herschel photometric observations of the nearby low metallicity irregular galaxy NGC 6822

M. Galametz, S. C. Madden, F. Galliano +57

We present the first Herschel PACS and SPIRE images of the low-metallicity galaxy NGC6822 observed from 70 to 500 mu and clearly resolve the HII regions with PACS and SPIRE. We fin…

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