activity
20102026
most citedThe physical properties of the dust in the RCW 120 HII region as seen by Herschel

70 citations · 110 across the 7 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2026

H2 emission in the Orion Bar, NGC7023 and the Horsehead Nebula observed with the James Webb Space Telescope

M. Zannese, A. Sidhu, A. Guerras +25

Molecular hydrogen (H2), the most abundant molecule in the interstellar medium, is a handy tool to study Photodissociation Regions. The JWST, with its high spatial resolution, sens…

astro-ph.GA2025

JWST observations of photodissociation regions III. Dust modelling at the illuminated edge of the Horsehead PDR

M. Elyajouri, A. Abergel, N. Ysard +19

Carbonaceous nano-grains are a significant component of interstellar dust and dominate the mid-infrared emission of photodissociation regions (PDRs). We study the evolution of nano…

astro-ph.GA2025

JWST observations of photodissociation regions: II. Warm molecular Hydrogen spectroscopy in the Horsehead nebula

M. Zannese, P. Guillard, A. Abergel +16

H2 is the most abundant molecule in the interstellar medium and is a useful tool to study photodissociation regions, where radiative feedback from massive stars on molecular clouds…

astro-ph.EP2024

MINDS. The DR Tau disk I: combining JWST-MIRI data with high-resolution CO spectra to characterise the hot gas

Milou Temmink, Ewine F. van Dishoeck, Sierra L. Grant +29

The MRS mode of the JWST-MIRI instrument has been shown to be a powerful tool to characterise the molecular gas emission of the inner region of planet-forming disks. Here, we analy…

astro-ph.GA2016★ 10 cited

Three-dimensional distribution of hydrogen fluoride gas toward NGC6334 I and I(N)

M. H. D. van der Wiel, D. A. Naylor, G. Makiwa +2

Aims. We investigate the spatial distribution of a collection of absorbing gas clouds, some associated with the dense, massive star-forming core NGC6334 I, and others with diffuse…

astro-ph.GA2015★ 5 cited

SPIRE-FTS observations of RCW 120

J. A. Rodón, A. Zavagno, J. -P. Baluteau +5

The expansion of Galactic HII regions can trigger the formation of a new generation of stars. However, little is know about the physical conditions that prevail in these regions. W…