activity
20172020
most citedDust absorption and scattering in the silicon K-edge

43 citations · 119 across the 3 of their papers we have counts for

collaborators

5 papers

astro-ph.HE202036 cited

Magnesium and silicon in interstellar dust: an X-ray overview

D. Rogantini, E. Costantini, S. T. Zeegers +5

The dense Galactic environment is a large reservoir of interstellar dust. Therefore, this region represents a perfect laboratory to study the properties of the cosmic dust grains.…

astro-ph.GA2019

Interstellar dust along the line of sight of GX 3+1

D. Rogantini, E. Costantini, S. T. Zeegers +6

Studying absorption and scattering of X-ray radiation by interstellar dust grains allows us to access the physical and chemical properties of cosmic grains even in the densest regi…

astro-ph.GA2019

X-ray extinction from interstellar dust: Prospects of observing carbon, sulfur and other trace elements

E. Costantini, S. T. Zeegers, D. Rogantini +3

We present a study on the prospects of observing carbon, sulfur, and other lower abundance elements (namely Al, Ca, Ti and Ni) present in the interstellar medium using future X-ray…

astro-ph.GA201943 cited

Dust absorption and scattering in the silicon K-edge

S. T. Zeegers, E. Costantini, D. Rogantini +5

The composition and properties of interstellar silicate dust are not well understood. In X-rays, interstellar dust can be studied in detail by making use of the fine structure feat…

astro-ph.HE201740 cited

Investigating the interstellar dust through the Fe K-edge

D. Rogantini, E. Costantini, S. T. Zeegers +5

The chemical and physical properties of interstellar dust in the densest regions of the Galaxy are still not well understood. X-rays provide a powerful probe since they can penetra…