Search Results - "van Hoof, Peter A M"
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Real-Time Stellar Evolution of Sakurai's Object
Published in Science (American Association for the Advancement of Science) (08-04-2005)“…After a hot white dwarf ceases its nuclear burning, its helium may briefly and explosively reignite. This causes the star to evolve back into a cool giant,…”
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JWST observations of the Ring Nebula (NGC 6720): I. Imaging of the rings, globules, and arcs
Published in Monthly notices of the Royal Astronomical Society (01-02-2024)“…ABSTRACT We present JWST images of the well-known planetary nebula NGC 6720 (the Ring Nebula), covering wavelengths from 1.6 to 25 $\, \mu$m. The bright shell…”
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Recent Development of the Atomic Line List
Published in Galaxies (01-06-2018)“…The Atomic Line List is an online database of wavelengths and transition probabilities of atomic lines. It is primarily set up as a tool to help identify…”
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Implications of Infalling Fe II-Emitting Clouds in Active Galactic Nuclei: Anisotropic Properties
Published in The Astrophysical journal (10-12-2009)“…We investigate consequences of the discovery that Fe II emission in quasars, one of the spectroscopic signatures of 'Eigenvector 1', may originate in infalling…”
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The Belgian Repository of Fundamental Atomic Data and Stellar Spectra (BRASS) Identifying Fruitful Methods for Producing Atomic Data
Published in Galaxies (01-09-2018)“…The Belgian repository of fundamental atomic data and stellar spectra (BRASS) aims to provide the largest systematic and homogeneous quality assessment to-date…”
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The Real-Time Evolution of V4334 Sgr
Published in Galaxies (01-09-2018)“…V4334 Sgr (Sakurai’s object) is an enigmatic evolved star that underwent a very late thermal pulse a few years before its discovery in 1996. It ejected a new…”
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The Belgian Repository of Fundamental Atomic Data and Stellar Spectra (BRASS)
Published in Atoms (2019)“…Background: BRASS (Belgian Repository of Fundamental Atomic Data and Stellar Spectra) is an international networking project for the development of a new…”
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Radio Continuum Spectra of Planetary Nebulae
Published in Galaxies (27-12-2018)“…Radio continuum emission of planetary nebulae is a rich source of information about their structure and physical parameters. Although radio emission is well…”
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Recombination of Hot Ionized Nebulae: The Old Planetary Nebula around V4334 Sgr (Sakurai’s Star)
Published in The Astrophysical journal (01-11-2022)“…Abstract After becoming ionized, low-density astrophysical plasmas will begin a process of slow recombination. Models for this still have significant…”
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The cooling-down central star of the planetary nebula SwSt 1: a late thermal pulse in a massive post-AGB star?
Published in Monthly notices of the Royal Astronomical Society (01-10-2020)“…ABSTRACT SwSt 1 (PN G001.5-06.7) is a bright and compact planetary nebula containing a late [WC]-type central star. Previous studies suggested that the nebular…”
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Herschel Planetary Nebula Survey (HerPlaNS)★: hydrogen recombination laser lines in Mz 3
Published in Monthly notices of the Royal Astronomical Society (11-07-2018)“…ABSTRACT The bipolar nebula Menzel 3 (Mz 3) was observed as part of the Herschel Planetary Nebula Survey (HerPlaNS), which used the PACS and SPIRE instruments…”
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First Images of the Molecular Gas around a Born-again Star Revealed by ALMA
Published in Astrophysical journal. Letters (01-01-2022)“…Abstract Born-again stars allow probing stellar evolution in human timescales and provide the most promising path for the formation of hydrogen-deficient…”
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Radiative cooling in collisionally ionized and photoionized plasmas
Published in Monthly notices of the Royal Astronomical Society (11-03-2013)“…We discuss recent improvements in the calculation of the radiative cooling in both collisionally ionized and photoionized plasmas. We are extending the…”
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Ultraviolet emission lines of Si ii in cool star and solar spectra
Published in Monthly notices of the Royal Astronomical Society (21-01-2016)“…Recent atomic physics calculations for Si II are employed within the CLOUDY modelling code to analyse Hubble Space Telescope (HST) STIS ultraviolet spectra of…”
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Non-thermal radio emission in Sakurai's Object
Published 25-07-2024“…A&A 688, L21 (2024) The very late thermal pulse (VLTP) affects the evolution of $\sim$20\% of 1--8\,$\mathrm M_\odot$ stars, repeating the last phases of the…”
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Recombination of hot ionized nebulae: The old planetary nebula around V4334 Sgr (Sakurai's star)
Published 08-09-2022“…After becoming ionized, low-density astrophysical plasmas will begin a process of slow recombination. Models for this still have significant uncertainties. The…”
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The cooling-down central star of the planetary nebula SwSt\,1: a late thermal pulse in a massive post-AGB star?
Published 30-09-2020“…2020, Volume 498, pp. 1205-1220 SwSt 1 (PN G001.5-06.7) is a bright and compact planetary nebula containing a late [WC]-type central star. Previous studies…”
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First images of the molecular gas around a born-again star revealed by ALMA
Published 11-01-2022“…Born-again stars allow probing stellar evolution in human timescales and provide the most promising path for the formation of hydrogen-deficient…”
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Properties of Dust Grains in Planetary Nebulae. I. The Ionized Region of NGC 6445
Published in The Astrophysical journal (20-03-2000)Get full text
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Radio observations of planetary nebulae: no evidence for strong radial density gradients
Published 03-07-2018“…Radio continuum observations trace thermal emission of ionized plasma in planetary nebulae and bring useful information on nebular geometries. A model of…”
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