The distance to Tycho's supernova remnant (3C 10) – a rediscussion

New H I observations of 3C10 at high velocity-resolution (1 km s−1) have been made with the Westerbork Synthesis Radio Telescope. H I absorption can be identified in the velocity range +8 to –52 km s−1. The resulting lower limit for the distance is 4 kpc; the systematic peculiar motions in the Perse...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 1980-09, Vol.192 (1), p.67P-71P
Hauptverfasser: Schwarz, U. J., Arnal, E. M., Goss, W. M.
Format: Artikel
Sprache:eng
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Zusammenfassung:New H I observations of 3C10 at high velocity-resolution (1 km s−1) have been made with the Westerbork Synthesis Radio Telescope. H I absorption can be identified in the velocity range +8 to –52 km s−1. The resulting lower limit for the distance is 4 kpc; the systematic peculiar motions in the Perseus arm have little effect on this determination. A weaker upper limit of 5 kpc has also been determined by a comparison with 3C 11.1, a nearby extragalactic source.
ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/192.1.67P