The Deep Rho Ophiuchi XMM-Newton Observation (DROXO)

Franco Palla, Testi, Damiani, Stelzer, Flaccomio, Montmerle, Ignazio Pillitteri, Giardino, Grosso, Favata, Sciortino, Palla, Micela, Ignazio Francesco Pillitteri

Risultato della ricerca: Other

3 Citazioni (Scopus)

Abstract

We present the X-ray data and the analysis status of the DROXO (Deep Rho Oph XMM-Newton Observation) project, aimed to mainly characterize the spectrovariability properties of YSOs in the nearby and very young p Oph star forming region. We focus on a few selected initial scientific results for few interesting YSOs, such as Elias 29 and YLWI 6A. In Elias 29 we see the 6.4 keV fluorescent Fe line as already reported in literature, whereas in YLW16A we do not detect the fluorescent line at odd with previous findings. Hence we conclude that the line intensity does change with time (and/or physical conditions).
Lingua originaleEnglish
Pagine111-112
Stato di pubblicazionePublished - 2006

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All Science Journal Classification (ASJC) codes

  • Aerospace Engineering
  • Space and Planetary Science

Cita questo

Palla, F., Testi, Damiani, Stelzer, Flaccomio, Montmerle, Pillitteri, I., Giardino, Grosso, Favata, Sciortino, Palla, Micela, & Pillitteri, I. F. (2006). The Deep Rho Ophiuchi XMM-Newton Observation (DROXO). 111-112.