activity
20102026
most citedThe complete far-infrared and submillimeter spectrum of the Class 0 protostar Serpens SMM1 obtained with Herschel. Characterizing UV-irradiated shocks heating and chemistry

89 citations · 320 across the 9 of their papers we have counts for

collaborators

10 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★ 5 cited

PDRs4All XV: CH radical and H molecular ion in the irradiated protoplanetary disk d203-506

I. Schroetter, O. Berné, J. R. Goicoechea +20

Most protoplanetary disks experience a phase in which they are subjected to strong ultraviolet radiation from nearby massive stars. This UV radiation can substantially alter their…

astro-ph.GA2024★ 9 cited

PDRs4All. V. Modelling the dust evolution across the illuminated edge of the Orion Bar

M. Elyajouri, N. Ysard, A. Abergel +31

We study the emission of dust grains within the Orion Bar - a well-known, highly far-UV (FUV)-irradiated PDR. The Orion Bar because of its edge-on geometry provides an exceptional…

astro-ph.GA2014★ 26 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.GA2013★ 25 cited

Kinematics of the ionized-to-neutral interfaces in Monoceros R2

P. Pilleri, A. Fuente, M. Gerin +10

Context. Monoceros R2 (Mon R2), at a distance of 830 pc, is the only ultra-compact H ii region (UC H ii) where its associated photon-dominated region (PDR) can be resolved with the…

astro-ph.GA2012★ 89 cited

The complete far-infrared and submillimeter spectrum of the Class 0 protostar Serpens SMM1 obtained with Herschel. Characterizing UV-irradiated shocks heating and chemistry

Javier R. Goicoechea, J. Cernicharo, A. Karska +8

We present the first complete 55-671 um spectral scan of a low-mass Class 0 protostar (Serpens SMM1) taken with the PACS and SPIRE spectrometers on board Herschel. More than 145 li…

astro-ph.GA2010★ 35 cited

Gas morphology and energetics at the surface of PDRs: new insights with Herschel observations of NGC 7023

C. Joblin, P. Pilleri, J. Montillaud +37

We investigate the physics and chemistry of the gas and dust in dense photon-dominated regions (PDRs), along with their dependence on the illuminating UV field. Using Herschel-HIFI…

astro-ph.GA2010★ 20 cited

The origin of the [C II] emission in the S140 PDRs - new insights from HIFI

C. Dedes, M. Röllig, B. Mookerjea +38

Using Herschel's HIFI instrument we have observed [C II] along a cut through S140 and high-J transitions of CO and HCO+ at two positions on the cut, corresponding to the externally…

astro-ph.GA2010★ 87 cited

Detection of interstellar oxidaniumyl: abundant H2O+ towards the star-forming regions DR21, Sgr B2, and NGC6334

V. Ossenkopf, H. S. P. Müller, D. C. Lis +99

We identify a prominent absorption feature at 1115 GHz, detected in first HIFI spectra towards high-mass star-forming regions, and interpret its astrophysical origin. The character…

astro-ph.GA2010★ 24 cited

HIFI observations of warm gas in DR21: Shock versus radiative heating

V. Ossenkopf, M. Röllig, R. Simon +35

The molecular gas in the DR21 massive star formation region is known to be affected by the strong UV field from the central star cluster and by a fast outflow creating a bright sho…