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High velocities in the new supernova remnant in Cygnus

Journal Article · · Sov. Astron. Lett. (Engl. Transl.); (United States)
OSTI ID:6287500
;
Interferometry of a bright region in the newly discovered Cygnus supernova remnant has been performed in the H..cap alpha.. line with a high-contrast Fabry--Perot etalon and a contact image tube. The gas in the remnant exhibits fast internal motions, reaching Vatsub LSRatl100 km/sec.
Research Organization:
Shternberg Astronomical Institute, Moscow
OSTI ID:
6287500
Journal Information:
Sov. Astron. Lett. (Engl. Transl.); (United States), Journal Name: Sov. Astron. Lett. (Engl. Transl.); (United States) Vol. 4:6; ISSN SALED
Country of Publication:
United States
Language:
English

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Related Subjects

640102* -- Astrophysics & Cosmology-- Stars & Quasi-Stellar
Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
BALMER LINES
COSMIC GASES
COSMIC RADIO SOURCES
ERUPTIVE VARIABLE STARS
FLUIDS
GASES
INTERFEROMETRY
STARS
SUPERNOVA REMNANTS
SUPERNOVAE
VARIABLE STARS
VELOCITY