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20032008
most citedRadio interferometric observations of candidate water-maser-emitting planetary nebulae

33 citations · 52 across the 2 of their papers we have counts for

collaborators

7 papers

astro-ph200833 cited

Radio interferometric observations of candidate water-maser-emitting planetary nebulae

Jose F. Gomez, Olga Suarez, Yolanda Gomez +4

We present Very Large Array (VLA) observations of H2O and OH masers, as well as radio continuum emission at 1.3 and 18 cm toward three sources previously cataloged as planetary neb…

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-ph2004

High-Resolution Observations in B1-IRS: ammonia, CCS and water masers

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

We present a study of the structure and dynamics of the star forming region B1-IRS (IRAS 03301+3057) using the properties of different molecules at high angular resolution (~4'').…

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…