Home News About Us Contact Contributors Disclaimer Privacy Policy Help FAQ

Home
Search
Quick Search
Advanced
Fulltext
Browse
Collections
Persons
My eDoc
Session History
Login
Name:
Password:
Documentation
Help
Support Wiki
Direct access to
document ID:


          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



ID: 742621.0, MPI für Astronomie / Publikationen_mpia
Balmer-dominated shocks in Tycho's SNR: omnipresence of CRs
Authors:Knežević, S.; Läsker, R.; van de Ven, G.; Font, J.; Raymond, J. C.; Bailer-Jones, C. A. L.; Beckman, J.; Morlino, G.; Ghavamian, P.; Hughes, J. P.; Heng, K.; Renaud, M.; Dubner, G.; Ray, A.; Bykov, A.
Place of Publication:Cambridge
Publisher:Cambridge Univ. Press
Date of Publication (YYYY-MM-DD):2017
Audience:Not Specified
Abstract / Description:We present wide-field, spatially and highly resolved spectroscopic observations of Balmer filaments in the northeastern rim of Tycho's supernova remnant in order to investigate the signal of cosmic-ray (CR) acceleration. The spectra of Balmer-dominated shocks (BDSs) have characteristic narrow (FWHM ~ 10 km s-1) and broad (FWHM ~ 1000 km s-1) Hα components. CRs affect the Hα-line parameters: heating the cold neutrals in the interstellar medium results in broadening of the narrow Hα-line width beyond 20 km s-1, but also in reduction of the broad Hα-line width due to energy being removed from the protons in the post-shock region. For the first time we show that the width of the narrow Hα line, much larger than 20 km s-1, is not a resolution or geometric effect nor a spurious result of a neglected intermediate (FWHM ~ 100 km s-1) component resulting from hydrogen atoms undergoing charge exchange with warm protons in the broad-neutral precursor. Moreover, we show that a narrow line width >> 20 km s-1 extends across the entire NE rim, implying CR acceleration is ubiquitous, and making it possible to relate its strength to locally varying shock conditions. Finally, we find several locations along the rim, where spectra are significantly better explained (based on Bayesian evidence) by inclusion of the intermediate component, with a width of 180 km s-1 on average.
Free Keywords:Tycho's SNR; Balmer-dominated shocks; CR precursor; broad-neutral precursor
External Publication Status:published
Document Type:Other
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:URL:http://adsabs.harvard.edu/abs/2017IAUS..331..248K
The scope and number of records on eDoc is subject to the collection policies defined by each institute - see "info" button in the collection browse view.