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researcher

V. Cracco

40 papers hereh-index 15805 citations60 works total

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

author position
  • first author3
  • middle author26
  • last author1

Across the 30 of 40 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA20
  • astro-ph.HE9
  • astro-ph.CO7
  • astro-ph.SR4

identity via Semantic Scholar / OpenAlex

activity
20092018
most citedProperties of flat-spectrum radio-loud Narrow-Line Seyfert 1 Galaxies

164 citations · 1k across the 39 of their papers we have counts for

collaborators
Showing 2013Show all

3 papers · 1 filter

astro-ph.CO2013

Are Boltzmann Plots of Hydrogen Balmer lines a tool for identifying a subclass of S1 AGN?

P. Rafanelli, S. Ciroi, V. Cracco +4

It is becoming clear that we can define two different types of nearby AGN belonging to the Seyfert 1 class (S1), on the basis of the match of the intensities of their Broad Balmer…

astro-ph.GA2013★ 2 cited

The optical emission lines of type 1 X-ray bright Active Galactic Nuclei

G. La Mura, M. Berton, S. Ciroi +3

A strong X-ray emission is one of the defining signatures of nuclear activity in galaxies. According to the Unified Model for Active Galactic Nuclei (AGN), both the X-ray radiation…

astro-ph.SR2013★ 35 cited

X-Ray Grating Observations of Recurrent Nova T Pyxidis During The 2011 Outburst

Benjamin M. Tofflemire, Marina Orio, Kim L. Page +5

The recurrent nova T Pyx was observed with the X-ray gratings of Chandra and XMM-Newton, 210 and 235 days, respectively, after the discovery of the 2011 April 14 outburst. The X-ra…

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