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J. Fabregat

5 papers hereh-index 350 citations6 works total

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

author position
  • middle author2

Across the 2 of 5 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3
  • astro-ph2
same name
  • J. Fabregat — 56 papers, h 31
  • J. Fabregat — 3 papers, h 1
  • J. Fabregat — 1 paper
  • J. Fabregat — 1 paper, h 2
  • J. Fabregat — 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
20072017
most citedPulsations in the late-type Be star HD 50209 detected by CoRoT

36 citations · 99 across the 5 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2017★ 3 cited

Photometric and spectroscopic variability of the B5IIIe star HD 171219

L. Andrade, E. Janot-Pacheco, M. Emilio +11

We analyzed the star HD 171219, one of the relatively bright Be stars observed in the seismo field of the CoRoT satellite, in order to determine its physical and pulsation characte…

astro-ph.SR2009★ 36 cited

Pulsations in the late-type Be star HD 50209 detected by CoRoT

P. D. Diago, J. Gutierrez-Soto, M. Auvergne +22

The presence of pulsations in late-type Be stars is still a matter of controversy. It constitutes an important issue to establish the relationship between non-radial pulsations and…

astro-ph.SR2009★ 2 cited

More on pulsating B-type stars in the Magellanic Clouds

P. D. Diago, J. Gutiérrez-Soto, J. Fabregat +1

We present here the results of our research for B-type pulsators in low metallicity environments, searching for short-term periodic variability in a large sample of B and Be stars…

astro-ph2007★ 29 cited

Pulsating B and Be stars in the Small Magellanic Cloud

P. D. Diago, J. Gutierrez-Soto, J. Fabregat +1

Context: Stellar pulsations in main-sequence B-type stars are driven by the kappa-mechanism due to the Fe-group opacity bump. The current models do not predict the presence of inst…

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