1.5k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR102 papers
- Instituto de Astrofísica de CanariasES96 papers
- Osservatorio Astronomico di PadovaIT93 papers
- Universidad de La LagunaES87 papers
- Millennium Institute of AstrophysicsCL83 papers
- Max Planck Institute for AstronomyDE80 papers
- European Southern ObservatoryCL75 papers
- Space Telescope Science InstituteUS68 papers
- University of La SerenaCL65 papers
- Universidad de AntofagastaCL64 papers
- Pontificia Universidad Católica de ChileCL62 papers
- University of PaduaIT59 papers
5 papers · 1 filter
The Chandra Planetary Nebula Survey (ChanPlaNS). II. X-ray Emission from Compact Planetary Nebulae
M. Freeman, R. Montez, J. H. Kastner +24
We present results from the most recent set of observations obtained as part of the Chandra X-ray observatory Planetary Nebula Survey (ChanPlaNS), the first comprehensive X-ray sur…
Investigating the radio-loud phase of broad absorption line quasars
G. Bruni, J. I. González-Serrano, M. Pedani +5
Broad absorption lines (BALs) are present in the spectra of ~20% of quasars (QSOs); this indicates fast outflows (up to 0.2c) that intercept the observer's line of sight. These QSO…
The planetary nebula IPHASXJ211420.0+434136 (Ou5): insights into common-envelope dynamical and chemical evolution
R. L. M. Corradi, P. Rodriguez-Gil, D. Jones +7
While analysing the images of the IPHAS H survey, we noticed that the central star of the candidate planetary nebula IPHASXJ211420.0+434136 (also named Ou5) was clearly variable…
PAH Formation in O-rich Planetary Nebulae
L. Guzman-Ramirez, E. Lagadec, D. Jones +2
Polycyclic aromatic hydrocarbons (PAHs) have been observed in O-rich planetary nebulae towards the Galactic Bulge. This combination of oxygen-rich and carbon-rich material, known a…
The post-common-envelope, binary central star of the planetary nebula Hen 2-11
David Jones, Henri M. J. Boffin, Brent Miszalski +3
We present a detailed photometric study of the central star system of the planetary nebula Hen 2-11, selected for study because of its low-ionisation filaments and bipolar morpholo…