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(Commissariat à l'Énergie Atomique et aux Énergies Alternatives), 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
A Reappraisal of The Habitability of Planets around M Dwarf Stars
|Astrobiology|2007|341