With the advent of high-energy-density (HED) experimental facilities, such as high-energy
lasers and fast Z-pinch, pulsed-power facilities, millimeter-scale quantities of matter can be …

We present maps at high spatial and spectral resolution in emission lines of CCH, cC 3 H 2,
C 4 H, 12 CO and C 18 O of the edge of the Horsehead nebula obtained with the IRAM …

FEEDBACK is a SOFIA (Stratospheric Observatory for Infrared Astronomy) legacy program
dedicated to study the interaction of massive stars with their environment. It performs a …

Massive stars can determine the evolution of molecular clouds by eroding and photo-
evaporating their surfaces with strong ultraviolet (UV) radiation fields. Moreover, UV …

We present a study of small carbon chains and rings in Photon Dominated Regions (PDRs)
performed at millimetre wavelengths. Our sample consists of the Horsehead nebula (B33) …

Context. Theoretical models and laboratory experiments show that CH 3 OH is efficiently
formed on cold grain surfaces through the successive hydrogenation of CO, forming HCO …

Context. Understanding the initial properties of star-forming material and how they affect the
star formation process is key. From an observational point of view, the feedback from young …

We present high angular resolution images of the H 2 1–0 S (1) line emission obtained with
the Son of ISAAC (SOFI) at the New Technology Telescope (NTT) of the Horsehead nebula …

Aims. We present spectroscopic observations obtained with the infrared Spitzer Space
Telescope, which provide insight into the H 2 physics and gas energetics in …

We present the first polarized dust emission measurements of the Horsehead Nebula,
obtained using the POL-2 polarimeter on the Submillimetre Common-User Bolometer Array …