96 citations · 239 across the 6 of their papers we have counts for
6 papers · 1 filter
Fitting spectral energy distributions of FMOS-COSMOS emission-line galaxies at z1.6: Star formation rates, dust attenuation, and [OIII]5007 emission-line luminosities
J. A. Villa-Vélez, V. Buat, P. Theulé +2
We perform SED fitting analysis on a COSMOS sample covering UV-to-FIR wavelengths with emission lines from the FMOS survey. The sample of 182 objects with H and [OIII]$\lambda50…
Polar dust obscuration in broad-line active galaxies from the XMM-XXL field
V. Buat, G. Mountrichas, G. Yang +6
Dust is observed in the polar regions of nearby AGN and it is known to contribute substantially to their mid-IR emission and to the obscuration of their UV to optical emission. We…
The gas, metal and dust evolution in low-metallicity local and high-redshift galaxies
Ambra Nanni, Denis Burgarella, Patrice Theulé +2
The chemical enrichment in the interstellar medium (ISM) of galaxies is regulated by several physical processes: stellar evolution, grain formation and destruction, galactic inflow…
Evidence of surface catalytic effect on cosmic dust grain analogues: the ammonia and carbon dioxide surface reaction
Alexey Potapov, Patrice Theulé, Cornelia Jäger +1
Surface chemistry on cosmic dust grains plays an important role in the formation of molecules at low temperatures in the interstellar and circumstellar environments. For the first…
SOLIS IV. Hydrocarbons in the OMC-2 FIR 4 region, a probe of energetic particle irradiation of the region
C. Favre, C. Ceccarelli, A. López-Sepulcre +16
We report new interferometric images of cyclopropenylidene, c-CH, towards the young protocluster OMC-2 FIR\,4. The observations were performed at 82 and 85 GHz with the NOr…
Seeds of Life in Space (SOLIS). III. Zooming into the methanol peak of the pre-stellar core L1544
Anna Punanova, Paola Caselli, Siyi Feng +41
Towards the pre-stellar core L1544, the methanol (CHOH) emission forms an asymmetric ring around the core centre, where CHOH is mostly in solid form, with a clear peak 4000…