Balmer Filaments in Tycho's Supernova Remnant: An Interplay between Cosmic-ray and Broad-neutral Precursors

We present H spectroscopic observations and detailed modeling of the Balmer filaments in the supernova remnant (SNR) Tycho (SN 1572). We used GH FaS (Galaxy H Fabry-Pérot Spectrometer) on the William Herschel Telescope with a 3 4 × 3 4 field of view, 0 2 pixel scale, and instr = 8.1 km s−1 resolutio...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
Veröffentlicht in:	The Astrophysical journal 2017-09, Vol.846 (2), p.167
Hauptverfasser:	Kne evi, Sladjana, Läsker, Ronald, van de Ven, Glenn, Font, Joan, Raymond, John C., Bailer-Jones, Coryn A. L., Beckman, John, Morlino, Giovanni, Ghavamian, Parviz, Hughes, John P., Heng, Kevin
Format:	Artikel
Sprache:	eng
Schlagworte:	ACCELERATION Astrophysics ASTROPHYSICS, COSMOLOGY AND ASTRONOMY Bayesian analysis Bins COMPARATIVE EVALUATIONS COMPUTERIZED SIMULATION Confidence intervals COSMIC RADIATION Cosmic ray protons Cosmic rays EMISSION Emissions Field of view Filaments GALAXIES H alpha line ISM: individual objects (Tycho) ISM: supernova remnants LINE BROADENING Line spectra Mathematical models Parameters Precursors PROTONS RESOLUTION SHOCK WAVES Space telescopes Statistical analysis Statistical inference Supernova SUPERNOVA REMNANTS TELESCOPES TEV RANGE VELOCITY
Online-Zugang:	Volltext bestellen
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Schreiben Sie den ersten Kommentar!