Cas A knot and filament proper motions

DOI

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.

Identifier
DOI http://doi.org/10.26093/cds/vizier.16130343
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/ApJ/613/343
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/613/343
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/613/343
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/ApJ/613/343
Provenance
Creator Delaney T.; Rudnick L.; Fesen R.A.; Jones T.W.; Petre R.; Morse J.A.
Publisher CDS
Publication Year 2005
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Cosmology; Galactic and extragalactic Astronomy; Interstellar medium; Natural Sciences; Physics