Direct observations of bipolar outflow from HM sagittae

S. P S Eyres, R. J. Cohen, R. J. Davis, H. T. Kenny, H. M. Lloyd, M. F. Bode, S. M. Dougherty

Allbwn ymchwil: Cyfraniad at gyfnodolynErthygladolygiad gan gymheiriaid

1 Dyfyniad (Scopus)

Crynodeb

We observed HM Sagittae with the Multi-Element Radio Linked Interferometer Network (MERLIN) at 6 cm and 18cm. We find non-thermal bipolar outflow in the eastwest direction, associated with optical emission lines, and thermal ridges to the north and south associated with the UV nebulosity detected by the HST.

Iaith wreiddiolSaesneg
Tudalennau (o-i)457-458
Nifer y tudalennau2
CyfnodolynAstrophysics and Space Science
Cyfrol224
Rhif cyhoeddi1-2
Dynodwyr Gwrthrych Digidol (DOIs)
StatwsCyhoeddwyd - Chwef 1995

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