G17.8 + 16.7: A new supernova remnant

G17.8 + 16.7: A new supernova remnant

Non-thermal radio emission is detected in the region of the gamma-ray source FHES J1723.5 - 0501. The emission has an approximately circular shape 0.8° in diameter. The observations confirm its nature as a new supernova remnant, G 17.8 + 16.7. We derive constraints on the source parameters using the...

Full description

Bibliographic Details
Main Authors: Araya, M., Hurley-Walker, Natasha, Quirós-Araya, S.
Format: Journal Article
Language:English
Published: OXFORD UNIV PRESS 2022
Subjects:
Science & Technology
Physical Sciences
Astronomy & Astrophysics
ISM: supernova remnants
gamma-rays: general
radio continuum: general
LARGE-AREA TELESCOPE
EXTENDED SOURCE
FERMI
CATALOG
EMISSION
CANDIDATES
SEARCH
HAWC
astro-ph.HE
Online Access:http://purl.org/au-research/grants/arc/FT190100231
http://hdl.handle.net/20.500.11937/91780

Internet

http://purl.org/au-research/grants/arc/FT190100231
http://hdl.handle.net/20.500.11937/91780

Similar Items