Neutral hydrogen in the neighborhood of the supernova remnant W 50

Details Neutral hydrogen in the neighborhood of the supernova remnant W 50 Neutral hydrogen in the neighborhood of the supernova remnant W 50

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986afz....25..287g&link_type=abstract

(Astrofizika, vol. 25, Sept.-Oct. 1986, p. 287-295) Astrophysics (ISSN 0571-7132), vol. 25, no. 2, March 1987, p. 518-523. Trans

Astronomy and Astrophysics

Astronomy

Hydrogen, Molecular Clouds, Radio Astronomy, Supernova Remnants, Carbon Dioxide, Interstellar Gas, Radial Velocity, Radio Interferometers

Scientific paper

Observations of neutral hydrogen at wavelength 21 cm in the neighborhood of the supernova remnant W 50, which contains the unique object SS 433, have been made with the RATAN-600 radio telescope with resolution 2 x 130 arcmin x 6.3 km/sec. At a radial velocity of about 34 km/sec (kinematic distance 3 kpc) a patchy HI cloud is found with outer diameter 65 pc and mass of about 30,000 solar masses. In addition, at radial velocity 69 km/sec (kinematic distances 5.0 or 10.7 kpc) there is a HI cloud without appreciable large-scale motions. Some models that could explain the connection between these objects and the observed HI clouds are considered.

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