activity
20032007
most citedA sensitive survey for water maser emission towards Bok globules using the Robledo 70m antenna

19 citations · 35 across the 3 of their papers we have counts for

collaborators

7 papers

astro-ph20077 cited

VLA observations of candidate high-mass protostellar objects at 7 mm

Guido Garay, Luis F. Rodriguez, Itziar de Gregorio-Monsalvo

We present radio continuum observations at 7 mm made using the Very Large Array towards three massive star forming regions thought to be in very early stages of evolution selected…

astro-ph20069 cited

High-resolution observations of water masers in Bok globules

I. de Gregorio-Monsalvo, J. F. Gomez, O. Suarez +4

We present Very Large Array observations at 1.3 cm of several water maser detections obtained by previous single-dish studies of Bok globules in the Clemens & Barvainis (1988; CB)…

astro-ph200619 cited

A sensitive survey for water maser emission towards Bok globules using the Robledo 70m antenna

Jose F. Gomez, Itziar de Gregorio-Monsalvo, Olga Suarez +1

We report the most sensitive water maser survey towards Bok globules to date, using NASA's 70m antenna in Robledo de Chavela (Spain). We observed 207 positions within the CB catalo…

astro-ph2005

CCS and NH3 emission associated with low-mass young stellar objects

I. de Gregorio-Monsalvo, J. F. Gomez, O. Suarez +3

In this work we present a sensitive and systematic single-dish survey of CCS emission (complemented with ammonia observations) at 1 cm, toward a sample of low- and intermediate-mas…

astro-ph2005

High-Resolution Molecular Line Observations of the Environment of the Class 0 Source B1-IRS

I. de Gregorio-Monsalvo, C. J. Chandler, J. F. Gomez +3

In this work we present VLA observations of the NH3, CCS, and H2O maser emission at 1 cm from the star forming region B1-IRS (IRAS 03301+3057) with ~ 5" (=1750 AU) of angular resol…

astro-ph2003

Molecular Line Emission from Accretion Disks Around YSOs

Itziar de Gregorio-Monsalvo, Jose F. Gomez, Paola D'Alessio

In this work we model the expected molecular emission from protoplanetary disks, modifying different physical parameters, such as dust grain size, mass accretion rate, viscosity, a…