activity
20012021
most citedNew detections of H2O masers in planetary nebulae and post-AGB stars using the Robledo-70m antenna

35 citations · 125 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2021★ 2 cited

The reactivation of water maser emission in the planetary nebula IRAS 18061--2505 through a born-again episode

L. F. Miranda, O. Suárez, L. Olguín +12

Water maser emitting planetary nebulae (HO-PNe) are believed to be among the youngest PNe. We present new optical narrow- and broad-band images, intermediate- and high-resoluti…

astro-ph.GA2012★ 3 cited

VISIR-VLT high resolution study of the extended emission of four obscured post-AGB candidates

M. W. Blanco, M. A. Guerrero, G. Ramos-Larios +4

The onset of the asymmetry of planetary nebulae (PNe) is expected to occur during the late Asymptotic Giant Branch (AGB) and early post-AGB phases of low- and intermediate-mass sta…

astro-ph.SR2012★ 26 cited

An updated catalog of OH-maser-emitting planetary nebulae

L. Uscanga, J. F. Gómez, O. Suárez +1

Aims. We studied the characteristics of planetary nebulae (PNe) that show both OH maser and radio continuum emission (hereafter OHPNe). These have been proposed to be very young PN…

astro-ph.SR2011

VISIR-VLT Images of the Water Maser Emitting Planetary Nebula K 3-35

Mónica W. Blanco, Martín A. Guerrero, Luis F. Miranda +2

K3-35 is an extremely young bipolar planetary nebula that contains a precessing bipolar jet and a small (radius 80 AU) water maser equatorial ring. We have obtained VISIR- VLT imag…

astro-ph.SR2011

Water maser emission in planetary nebulae

L. F. Miranda, O. Suárez, J. F. Gómez

Planetary Nebulae (PNe) evolve from Asymptotic Giant Branch (AGB) stars after a brief post-AGB phase. Water maser emission is characteristic of oxygen-rich AGB stars, is observed i…

astro-ph.SR2009★ 25 cited

Water maser detections in southern candidates to post-AGB stars and Planetary Nebulae

O. Suárez, J. F. Gómez, L. F. Miranda +4

We intended to study the incidence and characteristics of water masers in the envelopes of stars in the post-AGB and PN evolutionary stages. We have used the 64-m antenna in Parkes…