Neutral hydrogen in the direction of the Vela supernova remnant

We have carried out a study of the distribution and kinematics of the neutral hydrogen in the direction of the Vela supernova remnant (SNR). A field of 6°.8 × 5°.4 centered at l = 264°.1, b = -1°.6 was surveyed using the Parkes 64 m radio telescope (half-power beamwidth 14′.7 at 21 cm). Nearly 2300...

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Guardado en:
Detalles Bibliográficos
Publicado: 1998
Materias:
H I - ISM
Individual (Vela supernova remnant) - ISM
ISM
Structure - radio continuum - supernova remnants
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046256_v116_n2_p813_Dubner
http://hdl.handle.net/20.500.12110/paper_00046256_v116_n2_p813_Dubner
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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