Astronomy and Astrophysics, 488, pp. 667-674, http://dx.doi.org./10.1051/0004-6361:10080
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2008 (v1)Journal articleUploaded on: December 4, 2022
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2007 (v1)Journal article
Astronomy and Astrophysics, 475, pp. 243-250, http://dx.doi.org./10.1051/0004-6361:7625
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2011 (v1)Journal article
International audience
Uploaded on: December 3, 2022 -
June 6, 2011 (v1)Publication
Classical Be stars are hot non-supergiant stars surrounded by a gaseous circumstellar disk that is responsible for the observed IR-excess and emission lines. The influence of binarity on these phenomena remains controversial. delta Sco is a binary system whose primary suddently began to exhibit the Be phenomenon at the last periastron in 2000....
Uploaded on: December 3, 2022 -
2011 (v1)Journal article
International audience
Uploaded on: December 3, 2022 -
2011 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
September 30, 2011 (v1)Journal article
We report on near-IR interferometric observations of the outburst of the recurrent nova T Pyx. We obtained near-IR observations of T Pyx at dates ranging from t=2.37d to t=48.2d after the outburst, with the CLASSIC recombiner, located at the CHARA array, and with the PIONIER and AMBER recombiners, located at the VLTI array. These data are...
Uploaded on: December 4, 2022