activity
20162024
most citedInferring the three-dimensional distribution of dust in the Galaxy with a non-parametric method: Preparing for Gaia

38 citations · 67 across the 4 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2024★ 9 cited

3D structure of the Milky Way out to 10 kpc from the Sun. Catalogue of large molecular clouds in the Galactic Plane

Sara Rezaei Kh., Henrik Beuther, Robert A. Benjamin +4

Understanding the 3D structure of the Milky Way is a crucial step in deriving properties of the star-forming regions, as well as the Galaxy as a whole. We present a novel 3D map of…

astro-ph.GA2021★ 4 cited

The effect of viewing angle on the Kennicutt-Schmidt relation of the local molecular clouds

Jouni Kainulainen, Sara Rezaei Kh., Andri Spilker +1

The Gaia data give us an unprecedented view to the 3-dimensional (3D) structure of molecular clouds in the Solar neighbourhood. We study how the projected areas and masses of cloud…

astro-ph.GA2021★ 16 cited

The "Maggie" filament: Physical properties of a giant atomic cloud

J. Syed, J. D. Soler, H. Beuther +19

The atomic phase of the interstellar medium plays a key role in the formation process of molecular clouds. Due to the line-of-sight confusion in the Galactic plane that is associat…

astro-ph.HE2018

3D mapping of the neutral X-ray absorption in the local interstellar medium: The Gaia and XMM-Newton synergy

Efraín Gatuzz, S. Rezaei Kh., Timothy R. Kallman +4

We present a three-dimensional map of the hydrogen density distribution in the Galactic interstellar medium. The hydrogen equivalent column densities were obtained from the Explori…

astro-ph.GA2016★ 38 cited

Inferring the three-dimensional distribution of dust in the Galaxy with a non-parametric method: Preparing for Gaia

S. Rezaei Kh., C. A. L. Bailer-Jones, R. J. Hanson +1

We present a non-parametric model for inferring the three-dimensional (3D) distribution of dust density in the Milky Way. Our approach uses the extinction measured towards stars at…