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F. Palla

43 papers hereh-index 458.4k citations322 works total

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

author position
  • sole author1
  • first author6
  • middle author17
  • last author8

Across the 32 of 43 papers where every author was matched, so the position is known.

fields
  • astro-ph40
  • astro-ph.CO2
  • astro-ph.GA1
same name
  • F. Palla — 6 papers, h 120
  • F. Palla — 3 papers

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
19982011
most citedX-ray Emission from T Tauri Stars and the Role of Accretion: Inferences from the XMM-Newton Extended Survey of the Taurus Molecular Cloud

158 citations · 925 across the 19 of their papers we have counts for

collaborators
Showing 2003Show all

4 papers · 1 filter

astro-ph2003

IRAS 23385+6053: a candidate protostellar massive object

F. Fontani, R. Cesaroni, L. Testi +7

We present the results of a multi-line and continuum study towards the source IRAS 23385+6053,performed with the IRAM-30m telescope, the Plateau de Bure Interferometer, the Very La…

astro-ph2003

Long-term study of water masers associated with Young Stellar Objects. II: Analysis

J. Brand, R. Cesaroni, G. Comoretto +4

(Abridged) H2O masers in 14 SFRs have been monitored once every 2-3 months for up to 13 years. We investigate the dependence of the overall spectral morphology of the maser emissio…

astro-ph2003

Dispersion in the lifetime and accretion rate of T Tauri discs

Philip J. Armitage, Cathie J. Clarke, Francesco Palla

We compare evolutionary models for protoplanetary discs that include disc winds with observational determinations of the disc lifetime and accretion rate in Taurus. Using updated e…

astro-ph2003

Formation of the First Stars by Accretion

K. Omukai, F. Palla

The process of star formation from metal-free gas is investigated by following the evolution of accreting protostars with emphasis on the properties of massive objects. The main ai…

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