activity
20192025
most citedUltra-deep 31.0-50.3 GHz spectral survey of IRC+10216

38 citations · 92 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2025

CO observations in rotating circumbinary post-AGB disks

I. Gallardo Cava, J. Alcolea, H. Van Winckel +3

There is a group of post-AGB stars that are part of a binary system and that show a significant NIR excess. These systems are known to host disks with Keplerian or quasi-Keplerian…

astro-ph.SR2024

Continuum and molecular emission from the inner regions of the symbiotic system R Aquarii

M. Gómez-Garrido, V. Bujarrabal, J. Alcolea +3

Symbiotic systems often include an asymptotic giant branch (AGB) star and a hot compact companion, such as a white dwarf, that are in close interaction. Due to the intense ultravio…

astro-ph.SR2023★ 5 cited

The nebula around the binary post-AGB star 89 Herculis

I. Gallardo Cava, J. Alcolea, V. Bujarrabal +2

There is a class of binary post-asymptotic giant branch (post-AGB) stars that exhibit remarkable near-infrared (NIR) excess. These stars are surrounded by disks with Keplerian or q…

astro-ph.SR2022★ 10 cited

Chemistry of nebulae around binary post-AGB stars: A molecular survey of mm-wave lines

I. Gallardo Cava, V. Bujarrabal, J. Alcolea +2

Context. There is a class of binary post-asymptotic giant branch (post-AGB) stars that exhibit remarkable near-infrared (NIR) excess. Such stars are surrounded by Keplerian or quas…

astro-ph.GA2021★ 38 cited

Ultra-deep 31.0-50.3 GHz spectral survey of IRC+10216

J. R. Pardo, J. Cernicharo, B. Tercero +8

Context. IRC+10216, the carbon-rich envelope of the asymptotic giant branch (AGB) star CW Leo, is one of the richest molecular sources in the sky. Available spectral surveys below…

astro-ph.SR2021★ 28 cited

Keplerian disks and outflows in post-AGB stars: AC Herculis, 89 Herculis, IRAS 19125+0343, and R Scuti

I. Gallardo Cava, M. Gómez-Garrido, V. Bujarrabal +3

There is a class of binary post-AGB stars with a remarkable near-infrared excess that are surrounded by Keplerian or quasi-Keplerian disks and extended outflows composed of gas esc…

astro-ph.SR2019★ 11 cited

Circumstellar envelopes of semi-regular long-period variables: mass-loss rate estimates and general model-fitting of the molecular gas

J. J. Díaz-Luis, J. Alcolea, V. Bujarrabal +4

We aim to study the main properties of a volume-limited unbiased sample of well-characterized semi-regular variables (SRs) in order to clarify important issues, such as the formati…