activity
20082026
most citedThe 5.25 & 5.7 m Astronomical Polycyclic Aromatic Hydrocarbon Emission Features

61 citations · 184 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2026

PDRs4All XVIII. JWST-NIRCam Photometric properties of protoplanetary disks in the Orion Nebula Cluster

P. Amiot, O. Berné, I. Schroetter +10

We use the high angular resolution NIRCam images from the PDRs4All program, combined with those of GTO program 1256, to extract key properties of disks in the Orion Nebula Cluster.…

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.GA2015★ 15 cited

Herschel PACS and SPIRE spectroscopy of the Photodissociation Regions associated with S 106 and IRAS 23133+6050

D. J. Stock, M. G. Wolfire, E. Peeters +4

Photodissociation regions (PDRs) contain a large fraction of all of the interstellar matter in galaxies. Classical examples include the boundaries between ionized regions and molec…

astro-ph.GA2011★ 53 cited

Coupled Blind Signal Separation and Spectroscopic Database Fitting of the Mid Infrared PAH Features

M. J. F. Rosenberg, O. Berné, C. Boersma +2

The aromatic infrared bands (AIBs) observed in the mid infrared spectrum are attributed to Polycyclic Aromatic Hydrocarbons (PAHs). We observe the NGC 7023-North West (NW) PDR in t…

astro-ph2008★ 61 cited

The 5.25 & 5.7 m Astronomical Polycyclic Aromatic Hydrocarbon Emission Features

C. Boersma, A. L. Mattioda, C. W. Bauschlicher +3

Astronomical mid-IR spectra show two minor PAH features at 5.25 and 5.7 m (1905 and 1754 cm) that hitherto have been little studied, but contain information about th…

astro-ph2008★ 50 cited

The characteristics of the IR emission features in the spectra of Herbig Ae stars: Evidence for chemical evolution

C. Boersma, J. Bouwman, F. Lahuis +4

Herbig Ae/Be stars are a class of young pre-main sequence stellar objects of intermediate mass and are known to have varying amounts of natal cloud material still present in their…