activity
19982001
most citedThe aromatic infrared bands as seen by ISO-SWS: probing the PAH model

180 citations · 217 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph2001★ 180 cited

The aromatic infrared bands as seen by ISO-SWS: probing the PAH model

L. Verstraete, C. Pech, Claire Moutou +6

We discuss the Aromatic Infrared Band (AIB) profiles observed by ISO-SWS towards a number of bright interstellar regions where dense molecular gas is illuminated by stellar radiati…

astro-ph2000★ 2 cited

Excitation of H_2 and HD in shocks and PDRs

F. Bertoldi, B. T. Draine, D. Rosenthal +5

Photodissociation regions (PDRs) and shocks give rise to conspicuous emission from rotationally and vibrationally excited molecular hydrogen. This line emission has now been studie…

astro-ph2000★ 30 cited

ISO-SWS Observations of OMC-1: H_2 and Fine Structure Lines

Dirk Rosenthal, Frank Bertoldi, Siegfried Drapatz

Using the Short-Wavelength-Spectrometer on the Infrared Space Observatory (ISO), we obtained near- and mid-infrared spectra toward the brightest H_2 emission peak of the Orion OMC-…

astro-ph1999★ 4 cited

Infrared spectroscopy of young supernova remnants heavily interacting with the interstellar medium

E. Oliva, A. F. M. Moorwood, S. Drapatz +2

ISO spectral observations of the supernova remnant RCW103 are presented. This object is the prototype of relatively young remnants with fast shocks interacting with dense interstel…

astro-ph1998★ 1 cited

ISO-SWS spectroscopy of IC443 and the origin of the IRAS 12 and 25 micron emission from radiative supernova remnants

E. Oliva, D. Lutz, S. Drapatz +1

ISO-SWS spectral observations of the supernova remnant IC443 are presented. Like other radiative SNRs, this object is characterized by prominent line-emitting filaments and relativ…