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researcher

Y. Nazé

155 papers hereh-index 354.8k citations368 works total

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

author position
  • sole author4
  • first author50
  • middle author73
  • last author11

Across the 138 of 155 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR104
  • astro-ph28
  • astro-ph.HE11
  • astro-ph.IM8
  • physics.hist-ph2
  • astro-ph.GA1
same name
  • Y. Nazé — 26 papers, h 2
  • Y. Nazé — 3 papers, 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
20012026
most citedX-Ray Spectroscopy of Stars

277 citations · 4.5k across the 154 of their papers we have counts for

collaborators
Showing 2009Show all

4 papers · 1 filter

astro-ph.SR2009★ 25 cited

A new investigation of the binary HD 48099

L. Mahy, G. Rauw, F. Martins +5

With an orbital period of about 3.078 days, the double-lined spectroscopic binary HD 48099 is, still now, the only short-period O+O system known in the Mon OB2 association. Even th…

astro-ph.SR2009★ 30 cited

Optical spectroscopy of X-Mega targets in the Carina nebula - VII On the multiplicity of Tr 16-112, HD 93343 and HD 93250

G. Rauw, Y. Nazé, E. Fernández Lajús +4

We present the results of a spectroscopic monitoring campaign devoted to three O-type stars in the Carina nebula. We derive the full SB2 orbital solution of the binary system Tr 16…

astro-ph.SR2009★ 64 cited

Early-type stars in the young open cluster NGC 2244 and in the Mon OB2 association I. The multiplicity of O-type stars

L. Mahy, Y. Naze, G. Rauw +4

Aims. We present the results obtained from a long-term spectroscopic campaign devoted to the multiplicity of O-type stars in the young open cluster NGC2244 and in the Mon OB2 assoc…

astro-ph.SR2009★ 277 cited

X-Ray Spectroscopy of Stars

M. Guedel, Y. Naze

(abridged) Non-degenerate stars of essentially all spectral classes are soft X-ray sources. Low-mass stars on the cooler part of the main sequence and their pre-main sequence prede…

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