activity
20072021
most citedKinematics of the H2O masers at the centre of the PN K3-35

34 citations · 70 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2021

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.SR202010 cited

FLASHING: New high-velocity HO masers in IRAS 182860959

Hiroshi Imai, Yuri Uno, Daichi Maeyama +8

We discovered new high-velocity components of HO maser emission in one of the "water fountain" sources, IRAS~182860959, which has been monitored using the Nobeyama 45 m tele…

astro-ph.SR2018

Rapidly-evolving episodic outflow in IRAS 18113-2503: clues to the ejection mechanism of the fastest water fountain

Gabor Orosz, Jose F. Gomez, Hiroshi Imai +11

Water fountains are evolved stars showing early stages of collimated mass loss during transition from the asymptotic giant branch, providing valuable insight into the formation of…

astro-ph.SR2018

ALMA imaging of the nascent planetary nebula IRAS 15103-5754

Jose F. Gomez, Gilles Niccolini, Olga Suarez +5

We present continuum and molecular line (CO, CO, HCO) observations carried out with the Atacama Large Millimeter/submillimeter Array toward the "water fountain" star IRA…

astro-ph.SR201524 cited

Time-variable non-thermal emission in the planetary nebula IRAS 15103-5754

Olga Suarez, Jose F. Gomez, Philippe Bendjoya +6

The beginning of photoionization marks the transition between the post-Asymptotic Giant Branch (post-AGB) and planetary nebula (PN) phases of stars with masses < 8 M_sun. This crit…

astro-ph200834 cited

Kinematics of the H2O masers at the centre of the PN K3-35

L. Uscanga, Y. Gómez, A. C. Raga +5

We have studied the kinematics traced by the water masers located at the centre of the planetary nebula (PN) K3-35, using data from previous Very Large Array (VLA) observations. An…