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E. Tatulli

3 papers here

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

author position
  • first author1
  • middle author1

Across the 2 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph3

identity via Semantic Scholar / OpenAlex

most citedThe origin of hydrogen line emission for five Herbig Ae/Be stars spatially resolved by VLTI/AMBER spectro-interferometry

157 citations · 208 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph2008★ 157 cited

The origin of hydrogen line emission for five Herbig Ae/Be stars spatially resolved by VLTI/AMBER spectro-interferometry

S. Kraus, K. -H. Hofmann, M. Benisty +14

To trace the accretion and outflow processes around YSOs, diagnostic spectral lines such as the BrG 2.166 micron line are widely used, although due to a lack of spatial resolution,…

astro-ph2008★ 7 cited

VSI: the VLTI spectro-imager

F. Malbet, D. Buscher, G. Weigelt +51

The VLTI Spectro Imager (VSI) was proposed as a second-generation instrument of the Very Large Telescope Interferometer providing the ESO community with spectrally-resolved, near-i…

astro-ph2008★ 44 cited

Spatially resolving the hot CO around the young Be star 51 Ophiuchi

E. Tatulli, F. Malbet, F. Menard +6

51 Oph is one of the few young Be stars displaying a strong CO overtone emission at 2.3 microns in addition to the near infrared excess commonly observed in this type of stars. In…

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