activity
20162022
most citedTomography of the unique on-going jet in the planetary nebula NGC 2392

23 citations · 65 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2022★ 21 cited

The Planetary Nebula in the 500 Myr old Open Cluster M37

Vasiliki Fragkou, Quentin A. Parker, Albert A. Zijlstra +3

We report confirmation of a large, evolved, bipolar planetary nebula and its blue, white dwarf central star as a member of the ~500 Myr old Galactic open star cluster M37 (NGC 2099…

astro-ph.SR2022★ 7 cited

The common envelope origins of the fast jet in the planetary nebula M 3-38

J. S. Rechy-García, J. A. Toalá, M. A. Guerrero +3

We present the analysis of Multi-Espectrógrafo en GTC de Alta Resolución para Astronomía (MEGARA) high-dispersion integral field spectroscopic observations of the bipolar planetary…

astro-ph.SR2021★ 23 cited

Tomography of the unique on-going jet in the planetary nebula NGC 2392

M. A. Guerrero, S. Cazzoli, J. S. Rechy-Garcia +5

Jets (fast collimated outflows) are claimed to be the main shaping agent of the most asymmetric planetary nebula (PNe) as they impinge on the circumstellar material at late stages…

astro-ph.SR2017

Proper motions of the HH1 jet

A. C. Raga, B. Reipurth, A. Esquivel +9

We describe a new method for determining proper motions of extended objects, and a pipeline developed for the application of this method. We then apply this method to an analysis o…

astro-ph.GA2017★ 13 cited

The kinematical behaviour of ORLs and CELs in Galactic PNe

Miriam Peña, Francisco Ruiz-Escobedo, Jackeline S. Rechy-Garcia +1

The kinematics of the plasma in 14 PNe is analysed by measuring the expansion velocities (V) of different ions as derived from their collisionally excited lines (CELs) and…

astro-ph.GA2016★ 1 cited

The kinematical behavior of ORLs and CELs in PNe with [WC] central star

Miriam Pena, Francisco Ruiz-Escobedo, Jackeline Rechy-Garcıa +1

In Planetary Nebulae (PNe) and HII regions ionic abundances can be derived by using collisionally excited lines (CELs) or recombination lines (ORLs). Such abundances do not coincid…