activity
20072026
most citedRadio to gamma-ray variability study of blazar S5 0716+714

116 citations · 1.6k across the 50 of their papers we have counts for

collaborators

51 papers

astro-ph.SR2026

The Molecular Circumstellar Environments of Red Supergiants in Galactic Open Clusters

Mark A. Siebert, Elvire De Beck, Guillermo Quintana-Lacaci +4

We aim to expand the sample of RSGs with direct measurements of circumstellar gas through millimeter observations of two of the largest coeval RSG populations in the Galaxy: the op…

astro-ph.SR2026

The Last Gasps of a Dying Star: ALMA Observations of the Pre-Planetary Nebula IRAS 06530-0213

Raghvendra Sahai, Wouter Vlemmings, Guillermo Quintana-Lacaci +16

We present high angular-resolution () ALMA observations of millimeter-wave line and continuum emission (at and mm) in the pre-planetary ne…

astro-ph.SR2026

The formation radius of HCN in O-rich asymptotic giant branch stars

L. Marinho, J. P. Fonfría, M. Agúndez +3

Molecules detected in circumstellar envelopes around asymptotic giant branch (AGB) stars are generally well explained in terms of formation under chemical equilibrium in the stella…

astro-ph.SR2026

Chemistry in the High expansion-velocity C-rich evolved star AFGL2233. Isotopic ratios, peculiarities and evolutionary status

G. Quintana-Lacaci, M. Agúndez, L. Velilla-Prieto +4

High expansion velocity carbon stars (HVCs) are a rare class of evolved stars whose circumstellar envelopes (CSEs) combine C-rich chemistry with unusually high expansion velocities…

astro-ph.GA2025

The circumstellar environment around the extreme Galactic red supergiant NML Cygni: Dense, dusty, and asymmetric

E. De Beck, H. Andrews, G. Quintana-Lacaci +1

Supernova observations imply the presence of a dense and asymmetric circumstellar environment around SN Type II progenitors, whereas the mass loss from these progenitors, namely, r…

astro-ph.SR2025★ 1 cited

Exploring circumstellar chemistry in X-ray emitting AGB stars

J. Alonso-Hernández, C. Sánchez Contreras, M. Agúndez +5

Aims. Our goal is to characterize the chemistry and physical conditions of the circumstellar envelopes (CSEs) of Asymptotic Giant Branch (AGB) binary candidate stars with UV-excess…