activity
20102016
most citedCompression and ablation of the photo-irradiated cloud the Orion Bar

148 citations · 265 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA201629 cited

Spatial distribution of FIR rotationally excited CH+ and OH emission lines in the Orion Bar PDR

A. Parikka, E. Habart, J. Bernard-Salas +7

The abundance of CH+ and OH and excitation are predicted to be enhanced by the presence of vibrationally excited H2 or hot gas (~500-1000 K) in PDRs with high incident FUV radiatio…

astro-ph.GA2016148 cited

Compression and ablation of the photo-irradiated cloud the Orion Bar

Javier R. Goicoechea, J. Pety, S. Cuadrado +7

The Orion Bar is the archetypal edge-on molecular cloud surface illuminated by strong ultraviolet radiation from nearby massive stars. Owing to the close distance to Orion (about 1…

astro-ph.GA201624 cited

The first CO+ image: Probing the HI/H2 layer around the ultracompact HII region Mon R2

S. P. Trevino-Morales, A. Fuente, A. Sanchez-Monge +12

The CO+ reactive ion is thought to be a tracer of the boundary between a HII region and the hot molecular gas. In this study, we present the spatial distribution of the CO+ rotatio…

astro-ph.GA201426 cited

Physical structure of the photodissociation regions in NGC 7023. Observations of gas and dust emission with Herschel

M. Köhler, E. Habart, H. Arab +16

The determination of the physical conditions in molecular clouds is a key step towards our understanding of their formation and evolution of associated star formation. We investiga…

astro-ph.GA201438 cited

Deuteration around the ultracompact HII region Mon R2

S. P. Treviño-Morales, P. Pilleri, A. Fuente +13

The massive star-forming region Mon R2 hosts the closest ultra-compact HII region that can be spatially resolved with current single-dish telescopes. We used the IRAM-30m telescope…

astro-ph.IM2010

Fusion between ground- and space-based mid-infrared observations

O. Berne, A. G. G. M. Tielens, P. Pilleri +1

Mid-infrared astronomy (operating at wavelengths ranging from 2 to 25 m) has progressed significantly in the last decades, thanks to the improvement of detector techniques and t…