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S. Fabbri

4 papers hereh-index 8251 citations29 works total

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

author position
  • middle author4

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph2
  • astro-ph.GA1
  • astro-ph.SR1
same name
  • S. Fabbri — 6 papers, h 5
  • S. Fabbri — 4 papers, h 4
  • S. Fabbri — 1 paper, h 9
  • S. Fabbri — 1 paper, h 18

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
20072014
most citedThe First Empirical Mass Loss Law for Population II Giants

95 citations · 173 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2014★ 37 cited

An empirical mass-loss law for Population II giants from the Spitzer-IRAC survey of Galactic globular clusters

L. Origlia, F. R. Ferraro, S. Fabbri +4

The main aim of the present work is to derive an empirical mass-loss (ML) law for Population II stars in first and second ascent red giant branches. We used the Spitzer InfraRed Ar…

astro-ph.SR2010★ 27 cited

Dust is forming along the red giant branch of 47 TUC

Livia Origlia, Robert T. Rood, Sara Fabbri +4

We present additional evidence that dust is really forming along the red giant branch (RGB) of 47 Tuc at luminosities ranging from above the horizontal branch to the RGB-tip (Origl…

astro-ph2008★ 14 cited

Probing the Galactic Bulge with deep Adaptive Optics imaging: the age of NGC 6440

L. Origlia, S. Lena, E. Diolaiti +4

We present first results of a pilot project aimed at exploiting the potentiality of ground based adaptive optics imaging in the near infrared to determine the age of stellar cluste…

astro-ph2007★ 95 cited

The First Empirical Mass Loss Law for Population II Giants

Livia Origlia, Robert T. Rood, Sara Fabbri +3

Using the Spitzer IRAC camera we have obtained mid-IR photometry of the red giant branch stars in the Galactic globular cluster 47 Tuc. About 100 stars show an excess of mid-infrar…

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