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researcher

E. Schisano

38 papers hereh-index 364.7k citations178 works total

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

author position
  • middle author24
  • last author3

Across the 27 of 38 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA30
  • astro-ph.IM4
  • astro-ph.SR3
  • astro-ph.EP1
same name
  • E. Schisano — 11 papers
  • E. Schisano — 1 paper
  • E. Schisano — 1 paper

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
20152025
most citedProperties of Hi-GAL clumps in the inner Galaxy]{The Hi-GAL compact source catalogue. I. The physical properties of the clumps in the inner Galaxy (−71.0∘<ℓ<67.0∘)

201 citations · 1.1k across the 23 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

3 papers · 1 filter

astro-ph.SR2019

Dense cores and star formation in the giant molecular cloud Vela~C

F. Massi, A. Weiss, D. Elia +12

Context The Vela Molecular Ridge is one of the nearest (700 pc) giant molecular cloud (GMC) complexes hosting intermediate-mass (up to early B, late O stars) star formation, and is…

astro-ph.SR2019★ 24 cited

Evolution of young protoclusters embedded in dense massive clumps. A new grid of population synthesis SED models and a new set of L/M evolutionary tracks

S. Molinari, A. Baldeschi, T. P. Robitaille +8

A grid of 20 millions 3-1100μm SED models is presented for synthetic young clusters embedded in dense clumps. The models depend on four primary parameters: the clump mass M$_{clu…

astro-ph.SR2018

Extreme star formation in the Milky Way: Luminosity distributions of young stellar objects in W49A and W51

D. J. Eden, T. J. T. Moore, J. S. Urquhart +8

We have compared the star-formation properties of the W49A and W51 regions by using far-infrared data from the Herschel infrared Galactic Plane Survey (Hi-GAL) and 850-um observati…

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