activity
19952007
most citedISOGAL: A deep survey of the obscured inner Milky Way with ISO at 7 and 15 micron and with DENIS in the near-infrared

85 citations · 371 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph2007★ 71 cited

Water maser variability over 20 years in a large sample of star-forming regions: the complete database

M. Felli, J. Brand, R. Cesaroni +10

Context. Water vapor emission at 22 GHz from masers associated with star-forming regions is highly variable. Aims. We present a database of up to 20 years of monitoring of a sample…

astro-ph2006★ 26 cited

New signposts of massive star formation in the S235A-B region

Marcello Felli, Fabrizio Massi, Massimo Robberto +1

We report on new aspects of the star-forming region S235AB revealed through high-resolution observations at radio and mid-infrared wavelengths. Using the Very Large Array, we carri…

astro-ph2004★ 5 cited

Monitoring water masers in star-forming regions

J. Brand, R. Cesaroni, G. Comoretto +4

An overview is given of the analysis of more than a decade of H2O maser data from our monitoring program. We find the maser emission to generally depend on the luminosity of the YS…

astro-ph2004★ 24 cited

New light on the S235A-B star forming region

M. Felli, F. Massi, A. Navarrini +3

The S235A-B star forming region has been extensively observed in the past from the radio to the near-IR, but what was happening in the immediate surroundings of the water maser, pl…

astro-ph2003★ 46 cited

Long-term study of water masers associated with Young Stellar Objects. II: Analysis

J. Brand, R. Cesaroni, G. Comoretto +4

(Abridged) H2O masers in 14 SFRs have been monitored once every 2-3 months for up to 13 years. We investigate the dependence of the overall spectral morphology of the maser emissio…

astro-ph2003★ 85 cited

ISOGAL: A deep survey of the obscured inner Milky Way with ISO at 7 and 15 micron and with DENIS in the near-infrared

A. Omont, G. Gilmore, C. Alard +38

The ISOGAL project is an infrared survey of specific regions sampling the Galactic Plane selected to provide information on Galactic structure,stellar populations,stellar mass-loss…