activity
20022020
most citedHigh resolution observations of SiO masers: comparing the spatial distribution at 43 and 86 GHz

62 citations · 275 across the 18 of their papers we have counts for

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6 papers · 1 filter

astro-ph2008★ 3 cited

European VLBI Network observations of 6.7-GHz methanol masers in a candidate circumstellar disc

Lisa Harvey-Smith, Rebeca Soria-Ruiz

The first high-resolution (5 mas) VLBI observations of 6.7-GHz methanol masers in DR21(OH)N, a candidate circumstellar disc around a very young massive star, are presented. Previou…

astro-ph2007★ 19 cited

First images of 6.7-GHz methanol masers in DR21(OH) and DR21(OH)N

L. Harvey-Smith, R. Soria-Ruiz, A. Duarte-Cabral +1

The first images of 6.7-GHz methanol masers in the massive star-forming regions DR21(OH) and DR21(OH)N are presented. By measuring the shapes, radial velocities and polarization pr…

astro-ph2004

First VLBI mapping of a rare SiO isotopic substitution

R. Soria-Ruiz, F. Colomer, J. Alcolea +3

We report the first VLBI map of the 7 mm v=0 J=1-0 maser line of the 29-SiO isotopic substitution in the long period variable star IRC+10011. We have found that this maser emission…

astro-ph2004★ 62 cited

High resolution observations of SiO masers: comparing the spatial distribution at 43 and 86 GHz

R. Soria-Ruiz, J. Alcolea, F. Colomer +4

We present sub-milliarcsecond observations of SiO masers in the late-type stars IRC +10011 and Chi Cyg. We have used the NRAO Very Long Baseline Array (VLBA) to map the 43 GHz (v=1…

astro-ph2004★ 1 cited

Multi-transition VLBA observations of circumstellar SiO masers

R. Soria-Ruiz, F. Colomer, J. Alcolea +5

On this paper, we present simultaneous VLBA observations of the J=1-0 and J=2-1 rotational lines in the v=1 and v=2 vibrationally excited states of SiO (at 7 and 3 mm wavelengths).…

astro-ph2002

The Relative Spatial Distribution of SiO Masers in AGB Stars at 43 and 86 GHz

J. -F. Desmurs, R. Soria-Ruiz, F. Colomer +6

We present the first VLBI images of SiO masers in the circumstellar envelope of an S-type star obtained with the newly developed capabilities of the Very Long Baseline Array (VLBA)…