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researcher

D. Nelson

5 papers hereh-index 12 citations7 works total

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

author position
  • middle author3
  • last author2

Across the 5 of 5 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA4
  • astro-ph.IM1
same name
  • D. Nelson — 24 papers, h 59
  • D. Nelson — 6 papers, h 3
  • D. Nelson — 4 papers, h 4
  • D. Nelson — 1 paper, h 6
  • D. Nelson — 1 paper, 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

collaborators
Showing astro-ph.GAShow all

4 papers · 1 filter

astro-ph.GA2026

Turbulence in the multi-phase circumgalactic medium: bridging TNG50 and idealized kpc-scale simulations

Jonas Biba, Dylan Nelson

The circumgalactic medium (CGM) is the extended multi-phase gaseous halo surrounding a galaxy. To study how its dynamics are shaped by the interplay of radiative cooling and turbul…

astro-ph.GA2026

Studying the absorption signatures of H I Lyman-α in the warm-hot circumgalactic medium with TNG50

P. Aparicio Marcos, P. Richter, M. Sparre +2

In this study, we investigate the spectral signatures of neutral hydrogen Lyman-I^± absorption arising from the warm-hot gas component of the circumgalactic medium (CGM) around $z…

astro-ph.GA2026

Analysis of synthetic OVI absorption associated with galaxy groups in SIMBA and TNG50 simulations

Tanmay Singh, Sanchayeeta Borthakur, Dylan Nelson +2

We compare OVI absorption in synthetic spectra from galaxy groups in the SIMBA and TNG50 cosmological hydrodynamic simulations against those observed from the COS-IGrM survey. We s…

astro-ph.GA2025

Two Channels of Metal-Rich Compact Stellar System Formation: Starbursts under High Ram Pressure versus Tidal Stripping

Yuan Bian, Min Du, Victor P. Debattista +9

Most galaxies follow well-defined scaling relations of metallicity and stellar mass; however, some outliers at the low mass end of the observed galaxy population exhibit unusually…

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