Skip to content
Universidad del Mar SIBUMAR Descubridor Institucional UMAR
  • Inicio
  • Búsqueda avanzada
  • Explorar
  • Login
    • English
    • Deutsch
    • Español
    • Français
    • Italiano
Advanced
  • Dust Absorption towards Supernova Remnant W44
Cover Image

Dust Absorption towards Supernova Remnant W44

Fuente: arXiv
Saved in:
Bibliographic Details
Main Authors: Tu, Tian-Yu, Boogert, Adwin, Chen, Yang, He, Wenlang
Format: Preprint
Published: 2026
Subjects:
Astrophysics of Galaxies
Online Access:
Acceder al recurso
Tags: Add Tag
No Tags, Be the first to tag this record!
  • Cite this
  • Text this
  • Email this
  • Print
  • Export Record
    • Export to RefWorks
    • Export to EndNoteWeb
    • Export to EndNote
  • Save to List
  • Permanent link
  • Holdings
  • Description
  • Comments
  • Similar Items
  • Staff View

Internet

https://arxiv.org/abs/2604.07683

Similar Items

  • Shock and Cosmic Ray Chemistry Associated with the Supernova Remnant W28
    by: Tu, Tian-Yu, et al.
    Published: (2024)
  • On the Interpretation of Mid-Infrared Absorption Lines of Gas-Phase H$_2$O as Observed by JWST/MIRI
    by: Li, Jialu, et al.
    Published: (2024)
  • A Yebes W band Line Survey towards an Unshocked Molecular Cloud of Supernova Remnant 3C391: Evidence of Cosmic-Ray-Induced Chemistry
    by: Tu, Tian-Yu, et al.
    Published: (2024)
  • Supernova Ejecta with Crystalline Silicate Dust in the Supernova Remnant MSH 15-52
    by: Kim, Hyun-Jeong, et al.
    Published: (2023)
  • Observational Evidence of Dust Evolution in Supernova Remnants: Size Redistribution Toward Larger Grains in Early Sedov Phase
    by: Zhao, He, et al.
    Published: (2025)
Universidad del Mar
Universidad del MarSistema Bibliotecario de la Universidad del MarDescubridor Institucional UMARImplementación y desarrollo: Mtro. Carlos Alonso Albores Pérez
InicioBúsqueda avanzadaExplorar
Visitas al Descubridor: 33,245© 2026 Universidad del Mar