Determination of the gas-to-dust ratio in nearby dense clouds using X-ray absorption measurements
M. H. Vuong(Commissariat à l'Énergie Atomique et aux Énergies Alternatives), Hiroshi Ozawa(Université Joseph Fourier), T. Montmerle(Leiden University), Eric D. Feigelson(Pennsylvania State University), L. Verstraete(Université Paris Cité), N. Grosso(Centre National de la Recherche Scientifique)
Cited by 267
Related Papers
The<i>Swift</i>Gamma‐Ray Burst Mission
|The Astrophysical Journal|2004|4.2k
High-Energy Processes in Young Stellar Objects
|Annual Review of Astronomy and Astrophysics|1999|730
From T Tauri stars to protostars: Circumstellar material and young stellar objects in the rho Ophiuchi cloud
|The Astrophysical Journal|1994|496
The XMM-Newton extended survey of the Taurus molecular cloud (XEST)
|Astronomy and Astrophysics|2006|366
ISOCAM observations of the $\mathsf{\rho}$ Ophiuchi cloud: Luminosity and mass functions of the pre-main sequence embedded cluster
|Astronomy and Astrophysics|2001|295