Near-IR photometry of PMS stars in rho Oph (Natta+, 2006)

Physics

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Stars: Pre-Main Sequence, Accretion, Stars: Masses, Effective Temperatures, Photometry: Infrared, Equivalent Widths

Scientific paper

Near infrared moderate resolution J and K band spectroscopic observations of all targets in our sample were obtained at the ESO Observatories in Chile. The objects were either observed using the SofI instrument at the NTT 2.2m telescope (June 2004, Visitor Mode) or the ISAAC instrument at the Antu 8.2m VLT unit telescope (Spring 2004, Service Mode).
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