On the origin of [NeII] 12.81 <i>μ</i>m emission from pre-main sequence stars: Disks, jets, and accretion
M. Güdel(University of Vienna), E. F. van Dishoeck(Leiden University), R. van Boekel(Max Planck Institute for Astronomy), J. Carr(Centre de physique des particules de Marseille), A. E. Glassgold(University of California, Berkeley), Joan Najita(University of Arizona), K. R. Briggs(Paul Scherrer Institute), Th. Henning(Max Planck Institute for Astronomy), F. Lahuis(Leiden University)
Cited by 96
Related Papers
The ratio of the nucleon structure functions F2N for iron and deuterium
|Physics Letters B|1983|1.1k
ANTARES: The first undersea neutrino telescope
|Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment|2011|643
Hydrogenation reactions in interstellar CO ice analogues
|Astronomy and Astrophysics|2009|465
The XMM-Newton extended survey of the Taurus molecular cloud (XEST)
|Astronomy and Astrophysics|2006|366