High resolution monitoring of the emission lines in SS 433

Details High resolution monitoring of the emission lines in SS 433 High resolution monitoring of the emission lines in SS 433

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985msngr..42...17a&link_type=abstract

ESO Messenger (ISSN 0722-6691), Dec. 1985, p. 17-20.

Astronomy and Astrophysics

Astronomy

Black Holes (Astronomy), Emission Spectra, Neutron Stars, Stellar Spectra, X Ray Binaries, High Resolution, Radio Sources (Astronomy), Spectral Resolution, Very Long Base Interferometry

Scientific paper

The star 433 of the Stephenson Sanduleak catalog of emission-line objects has now become one of the most intensively observed sources in the Galaxy. There is evidence that SS 433 is an X-ray binary whose compact component is either a neutron star or a black hole. An investigation has been conducted with the objective to relate the changing details in the H-alpha profile to the moving blobs in the radio jet, taking into account an employment of the Caspec echelle spectrograph on a 3.6 m telescope to monitor the spectrum of SS 433 simultaneously with VLBI measurements of the radio structure. Attention is given to the purpose of the high spectral resolution, preliminary results from the Caspec data, and the results which can be expected from a comparison of optical and VLBI data.

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