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F. Massi

66 papers hereh-index 262.2k citations143 works total

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

author position
  • first author2
  • middle author40
  • last author6

Across the 48 of 66 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR26
  • astro-ph17
  • astro-ph.GA15
  • astro-ph.IM6
  • astro-ph.EP2
same name
  • F. Massi — 5 papers, h 4
  • F. Massi — 1 paper
  • F. Massi — 1 paper, h 1

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
20022026
most citedClouds, filaments and protostars: the Herschel Hi-GAL Milky Way

806 citations · 2.8k across the 65 of their papers we have counts for

collaborators
Showing 2009Show all

3 papers · 1 filter

astro-ph.GA2009★ 29 cited

The BLAST Survey of the Vela Molecular Cloud: Physical Properties of the Dense Cores in Vela-D

Luca Olmi, Peter A. R. Ade, Daniel Angles-Alcazar +34

The Balloon-borne Large-Aperture Submillimeter Telescope (BLAST) carried out a 250, 350 and 500 micron survey of the galactic plane encompassing the Vela Molecular Ridge, with the…

astro-ph.SR2009★ 13 cited

Resolving the asymmetric inner wind region of the yellow hypergiant IRC+10420 with VLTI/AMBER in low and high spectral resolution mode

T. Driebe, J. H. Groh, K. -H. Hofmann +15

We obtained near-infrared long-baseline interferometry of IRC+10420 with the AMBER instrument of ESO's Very Large Telescope Interferometer (VLTI) in low and high spectral resolutio…

astro-ph.GA2009★ 28 cited

The stellar population and complex structure of the bright-rimmed cloud IC 1396N

M. T. Beltran, F. Massi, R. Lopez +2

Context. IC 1396N is a bright-rimmed cloud associated with an intermediate-mass star-forming region, where a number of Herbig-Haro objects, H2 jet-like features, CO molecular outfl…

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