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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.COShow all

3 papers · 1 filter

astro-ph.CO2012★ 2 cited

Central regions of LIRGs: rings, hidden starbursts, Supernovae and star clusters

Petri Vaisanen, Andres Escala, Erkki Kankare +7

We study star formation (SF) in very active environments, in luminous IR galaxies, which are often interacting. A variety of phenomena are detected, such as central starbursts, cir…

astro-ph.CO2011

The nuclear PAH emission of merger system NGC 1614: rings within rings

Petri Vaisanen, Vinesh Rajpaul, Albert A. Zijlstra +2

It is important to understand the interplay between nuclear star-formation and nuclear activity when studying the evolution of gas rich galaxy mergers. We present here new spatiall…

astro-ph.CO2011★ 21 cited

The Spitzer discovery of a galaxy with infrared emission solely due to AGN activity

S. Hony, F. Kemper, Paul M. Woods +14

We present a galaxy (SAGE1CJ053634.78-722658.5) at a redshift of 0.14 of which the IR is entirely dominated by emission associated with the AGN. We present the 5-37 um Spitzer/IRS…

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