Hostname: page-component-77c89778f8-vpsfw Total loading time: 0 Render date: 2024-07-16T17:22:43.723Z Has data issue: false hasContentIssue false
  • English
  • Français

VLBA Observations of GRS 1915+105

Published online by Cambridge University Press:  12 April 2016

V. Dhawan ,
I. F. Mirabel  and
L. F. Rodríguez
V. Dhawan
Affiliation:
National Radio Astronomy Observatory, Socorro, NM 87801, U.S.A.
I. F. Mirabel
Affiliation:
Service d’Astrophysique, Saclay, F-91191 Gif-sur-Yvette, France
L. F. Rodríguez
Affiliation:
Instituto de Astronomia, UNAM, postal 70-264, 04510, Mexico

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

During quasi-periodic flux variations, the core of this galactic superluminal source shows: (a) a flat radio spectrum between 13cm and 2cm; (b) elongation of the core along the axis of arcsecond-scale ejecta; (c) a time-delay of ~4 mins at 3.6cm, relative to 2cm; (d) progressively less variation of the flux at 2cm, 3.6cm & 13cm; and (e) scatter-broadening to 1.9mas at 8.4GHz (135mas at 1GHz).

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 341 - 342
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Castro-Tirado, A.J. et al., 1994. ApJS, 92, 469–472.Google Scholar
Diamond, P.J. et al. 1988. Radio Wave Scattering in the Interstellar Medium, eds. Cordes, J.M., Rickett, B.J., & Backer, D.C., (New York: AIP), 174, 195–198.Google Scholar
Hjellming, R.M., & Johnston, K.J. 1988. ApJ, 328, 600–609.Google Scholar
Mirabel, I.F., & Rodriguez, L.F. 1994. Nature, 371, 46–48.Google Scholar
Rodríguez, L.F. et al. 1995. ApJS, 101, 173–179.Google Scholar
Rodríguez, L.F., & Mirabel, I.F. 1997. ApJ, 474, L123–126.Google Scholar