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researcher

A. Zijlstra

259 papers hereh-index 5410.5k citations584 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author9
  • first author10
  • middle author135
  • last author77

Across the 231 of 259 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR115
  • astro-ph101
  • astro-ph.GA36
  • astro-ph.CO3
  • astro-ph.HE3
  • astro-ph.IM1
same name
  • A. Zijlstra — 52 papers, h 4
  • A. Zijlstra — 15 papers, h 11
  • A. Zijlstra — 11 papers, h 2
  • A. Zijlstra — 6 papers, h 8
  • A. Zijlstra — 2 papers, h 9
  • A. Zijlstra — 2 papers, h 2

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
19932025
most citedAn empirical formula for the mass-loss rates of dust-enshrouded red supergiants and oxygen-rich Asymptotic Giant Branch stars

410 citations · 10k across the 259 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

3 papers · 1 filter

astro-ph.HE2023

A new method for short duration transient detection in radio images: Searching for transient sources in MeerKAT data of NGC 5068

S. Fijma, A. Rowlinson, R. A. M. J. Wijers +12

Transient surveys are a vital tool in exploring the dynamic universe, with radio transients acting as beacons for explosive and highly energetic astrophysical phenomena. However, p…

astro-ph.HE2021

The remnant and origin of the historical supernova 1181AD

Andreas Ritter, Quentin Parker, Foteini Lykou +3

The guest star of AD 1181 is the only historical supernova of the last millennium that is without a definite counterpart. The previously proposed association with supernova remnant…

astro-ph.HE2009★ 37 cited

Swift X-ray and UV monitoring of the Classical Nova V458 Vul (Nova Vul 2007)

J. -U. Ness, J. J. Drake, A. P. Beardmore +18

We describe the highly variable X-ray and UV emission of V458 Vul (Nova Vul 2007), observed by Swift between 1 and 422 days after outburst. Initially bright only in the UV, V458 Vu…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.