◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

Iraj Vaezzadeh

3 papers here

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

author position
  • middle author3

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE2
  • astro-ph.GA1
ORCID 0000-0002-0887-1236
same name
  • Iraj Vaezzadeh — 2 papers

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

most citedA toy model for gas sloshing in galaxy clusters

5 citations · 6 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2025

Mapping the Nearest Ancient Sloshing Cold Front in the Sky with XMM-Newton

Sheng-Chieh Lin, Yuanyuan Su, Iraj Vaezzadeh +8

The Virgo Cluster is the nearest cool core cluster that features two well-studied sloshing cold fronts at radii of r≈30 kpc and r≈90 kpc, respectively. In this…

astro-ph.HE2024★ 1 cited

How do supernova remnants cool? II. Machine learning analysis of supernova remnant simulations

P. Smirnova, E. I. Makarenko, S. D. Clarke +4

About 15%-60% of all supernova remnants are estimated to interact with dense molecular clouds. In these high density environments, radiative losses are significant. The cooling rad…

astro-ph.GA2024★ 5 cited

A toy model for gas sloshing in galaxy clusters

Elke Roediger, Iraj Vaezzadeh, Paul Nulsen

We apply a toy model based on 'pendulum waves' to gas sloshing in galaxy clusters. Starting with a galaxy cluster potential filled with a hydrostatic intra-cluster medium (ICM), we…

◍wovepaper

Papers, researchers and institutions, woven together.

Explore
  • Search
  • Researchers
  • Institutions
Account
  • Library
  • Chat
Data
  • arXiv.org
  • Semantic Scholar
  • OpenAlex
  • Latest RSS
AboutContactPrivacyDevelopersllms.txtopenapi.json
Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.