activity
20152023
most citedMUSE spectroscopy of planetary nebulae with high abundance discrepancies

38 citations · 175 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2023

Disk and Envelope Streamers of the GGD27-MM1 Massive Protostar

M. Fernández-López, J. M. Girart, J. A. López-Vázquez +4

We present new Atacama Large (sub)Millimeter Array 0.98 mm observations of the continuum emission and several molecular lines toward the high-mass protostellar system GGD27-MM1, dr…

astro-ph.SR2021★ 38 cited

MUSE spectroscopy of planetary nebulae with high abundance discrepancies

Jorge García-Rojas, Christophe Morisset, David Jones +5

We present MUSE deep integral-field unit spectroscopy of three planetary nebulae(PNe) with high abundance discrepancy factors (ADF > 20): NGC 6778, M 1-42 and Hf 2-2. We have const…

astro-ph.SR2021★ 29 cited

The HD 98800 quadruple pre-main sequence system. Towards full orbital characterisation using long-baseline infrared interferometry

S. Zúñiga-Fernández, J. Olofsson, A. Bayo +8

HD 98800 is a young ( Myr old) and nearby ( pc) quadruple system, composed of two spectroscopic binaries orbiting around each other (AaAb and BaBb), with a gas-rich…

astro-ph.HE2019★ 16 cited

The Palomar Transient Factory Sky2Night programme

J. van Roestel, P. J. Groot, T. Kupfer +9

We present results of the Sky2Night project: a systematic, unbiased search for fast optical transients with the Palomar Transient Factory. We have observed 407 deg in -band…

astro-ph.SR2018★ 24 cited

Spectro-interferometric observations of a sample of Be stars. Setting limits to the geometry and kinematics of stable Be disks

Y. R. Cochetti, C. Arcos, S. Kanaan +3

Be stars are rapid rotators surrounded by a gaseous disk envelope whose origin is still under debate. This envelope is responsible for observed emission lines and large infrared ex…

astro-ph.EP2018★ 4 cited

Is there really a debris disc around ?

V. Faramaz, G. Bryden, K. R. Stapelfeldt +10

The presence of a debris disc around the Gyr-old solar-type star was suggested by the infrared excess detection. Follow-up observations…

astro-ph.GA2018★ 25 cited

Primordial Mass and Density Segregation in a Young Molecular Cloud

Emilo J. Alfaro, Carlos Román-Zúñiga

We analyse the geometry of the Pipe Nebula, drawn by the distribution (-spatial parameter) and hierarchy ( spatial segregation) of column density peaks previously detected an…

astro-ph.SR2016★ 20 cited

Massive open star clusters using the VVV survey V. Young clusters with an OB stellar population

S. Ramírez Alegría, J. Borissova, A. -N. Chené +6

The ESO public survey VISTA Variables in the Vía Láctea (VVV) has contributed with deep multi-epoch photometry of the Galactic bulge and the adjacent part of the disk over 526 squa…

astro-ph.GA2015★ 17 cited

HERschel Observations of Edge-on Spirals (HEROES). II: Tilted-ring modelling of the atomic gas disks

F. Allaert, G. Gentile, M. Baes +9

Context. Edge-on galaxies can offer important insights in galaxy evolution as they are the only systems where the distribution of the different components can be studied both radia…

astro-ph.GA2015★ 2 cited

San Pedro Martir observations of microvariability in obscured quasars

Jana Polednikova, Alessandro Ederoclite, Jordi Cepa +9

Fast brightness variations are a unique tool to probe the innermost regions of active galactic nuclei (AGN). These variations are called microvariability or intra-night variability…