Cas A knot and filament proper motions Virtual Observatory Resource

Authors

1. Delaney T.
2. Rudnick L.
3. Fesen R.A.
4. Jones T.W.
5. Petre R.
6. Morse J.A.

Published by

CDS

Abstract

We present high-resolution X-ray proper-motion measurements of Cassiopeia A using Chandra X-Ray Observatory observations from 2000 and 2002. We separate the emission into four spectrally distinct classes: Si-dominated, Fe-dominated, low-energy-enhanced, and continuum-dominated. These classes also represent distinct spatial and kinematic components.

Keywords

1. supernova-remnants
2. proper-motions
3. x-ray-sources

Bibliographic source Bibcode

2004ApJ...613..343D

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/613/343

IVOA Identifier IVOID

ivo://CDS.VizieR/J/ApJ/613/343

Document Object Identifer DOI

doi:10.26093/cds/vizier.16130343

Access

Web browser access HTML

https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/613/343
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/613/343
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/613/343

IVOA Table Access TAP

https://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).