activity
20122021
most citedA New Radio Molecular Line Survey of Planetary Nebulae: HNC/HCN as a Diagnostic of Ultraviolet Irradiation

34 citations · 109 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2021

Multi-frequency high spectral resolution observations of HCN toward the circumstellar envelope of Y CVn

J. P. Fonfría, E. J. Montiel, J. Cernicharo +7

High spectral resolution observations toward the low mass-loss rate C-rich, J-type AGB star Y CVn have been carried out at 7.5, 13.1 and 14.0 um with SOFIA/EXES and IRTF/TEXES. Aro…

astro-ph.SR202018 cited

The post-common-envelope binary central star of the planetary nebula ETHOS 1

James Munday, David Jones, Jorge García-Rojas +7

We present a detailed study of the binary central star of the planetary nebula ETHOS 1 (PN G068.1+11.0). Simultaneous modelling of light and radial velocity curves reveals the bina…

astro-ph.SR2019

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…

astro-ph.SR201934 cited

A New Radio Molecular Line Survey of Planetary Nebulae: HNC/HCN as a Diagnostic of Ultraviolet Irradiation

Jesse Bublitz, Joel H. Kastner, Miguel Santander-García +3

Certain planetary nebulae contain shells, filaments, or globules of cold gas and dust whose heating and chemistry are likely driven by UV and X-ray emission from their central star…

astro-ph.SR2018

The short orbital period binary star at the heart of the planetary nebula M 3-1

David Jones, Henri M. J. Boffin, Paulina Sowicka +4

We present the discovery of a 3h5m orbital-period binary star at the heart of the planetary nebula M 3-1 - the shortest period photometrically-variable central star known and secon…

astro-ph.SR201728 cited

The planetary nebula IC 4776 and its post-common-envelope binary central star

Paulina Sowicka, David Jones, Romano L. M. Corradi +5

We present a detailed analysis of IC 4776, a planetary nebula displaying a morphology believed to be typical of central star binarity. The nebula is shown to comprise a compact hou…