Quantitative measurements of line intensities have been made since the beginning of the last century. The quantity and quality of the data available have increased drastically with the advent of electronic detectors. ...

In this work are presented measurements of the electron temperature in the HII region 30 Doradus derived from the [OIII](λ4959 + λ5007)/λ4363 ratio. Long-slit spectrophotometric data of high signal-to-noise, in the range ...

Context. We present the analysis of ISOCAM-CVF and the J, H, and K-s photometry data for the HII region complex N4 in the Large Magellanic Cloud (LMC). Aims. The aim is twofold: 1) to study the connection between the ...

We present high angular and spectral resolution Hi 21 cm line observations toward the cometary-shaped compact Hii region G213.880−11.837 in the GGD 14 complex. The kinematics and morphology of the photodissociated region, ...

We present a multiwavelength study of the interstellar medium around the HII region Sh2-54. The millimetric and infrared data allow us to analyze and characterize the molecular gas and dust components, respectively. The ...

Aims. As part of a systematic study that we are performing to increase the observational evidence of triggered star formation in the surroundings of HII regions, we analyze the ISM around the HII region G35.673-00.847, a ...

We present evidence for anomalous microwave emission in the RCW175 \hii region. Motivated by 33 GHz $13\arcmin$ resolution data from the Very Small Array (VSA), we observed RCW175 at 31 GHz with the Cosmic Background Imager ...

We present new echelle spectrophotometry of the Galactic H II regions M8 and M17. The data have been taken with the VLT UVES echelle spectrograph in the 3100 to 10400 A range. We have measured the intensities of 375 and ...