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researcher

A. Scholz

55 papers hereh-index 211.3k citations74 works total

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

author position
  • sole author3
  • first author10
  • middle author30
  • last author4

Across the 47 of 55 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR41
  • astro-ph.EP5
  • astro-ph.GA4
  • astro-ph3
  • astro-ph.IM2
same name
  • A. Scholz — 56 papers, h 30
  • A. Scholz — 16 papers, h 1
  • A. Scholz — 12 papers, h 3
  • A. Scholz — 9 papers, h 3
  • A. Scholz — 8 papers, h 9
  • A. Scholz — 6 papers, h 3

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
20032023
most citedTemperaments of young stars: Rapid mass-accretion rate changes in T Tauri and Herbig Ae stars

130 citations · 1.7k across the 55 of their papers we have counts for

collaborators
Showing 2017Show all

3 papers · 1 filter

astro-ph.SR2017★ 20 cited

Very Low-Mass Stars and Brown Dwarfs in Upper Scorpius using Gaia DR1: Mass Function, Disks and Kinematics

Neil J. Cook, Aleks Scholz, Ray Jayawardhana

Our understanding of the brown dwarf population in star forming regions is dependent on knowing distances and proper motions, and therefore will be improved through the Gaia space…

astro-ph.SR2017★ 31 cited

The JCMT Transient Survey: Identifying Submillimetre Continuum Variability over Several Year Timescales Using Archival JCMT Gould Belt Survey Observations

Steve Mairs, Doug Johnstone, Helen Kirk +19

Investigating variability at the earliest stages of low-mass star formation is fundamental in understanding how a protostar assembles mass. While many simulations of protostellar d…

astro-ph.SR2017★ 68 cited

How do stars gain their mass? A JCMT/SCUBA-2 Transient Survey of Protostars in Nearby Star Forming Regions

Gregory J. Herczeg, Doug Johnstone, Steve Mairs +55

Most protostars have luminosities that are fainter than expected from steady accretion over the protostellar lifetime. The solution to this problem may lie in episodic mass accreti…

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