A 408 MHz Survey of the Galactic Anticentre Region

The 250-foot aperture Mark I radio telescope at Jodrell Bank has been used to make a 408 MHz continuum survey of the Galactic anticentre region. The telescope resolution was 45 arc minutes. The region surveyed was $04 \,\text{h}. \lt \,\text{R.A.} \lt 12 \,\text{h.}, -20^{\circ} \lt \,\text{Dec}. \l...

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Veröffentlicht in:Mon. Notic. Roy. Astron. Soc. 147: 405-41(1970) 1970-04, Vol.147 (4), p.405-441
Hauptverfasser: Haslam, C. G. T., Quigley, M. J. S., Salter, C. J.
Format: Artikel
Sprache:eng
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Zusammenfassung:The 250-foot aperture Mark I radio telescope at Jodrell Bank has been used to make a 408 MHz continuum survey of the Galactic anticentre region. The telescope resolution was 45 arc minutes. The region surveyed was $04 \,\text{h}. \lt \,\text{R.A.} \lt 12 \,\text{h.}, -20^{\circ} \lt \,\text{Dec}. \lt + 60^{\circ}$ and $00 \,\text{h}. \lt \,\text{R.A.} \lt 04 \,\text{h.}, +20^{\circ} \lt \,\text{Dec}. \lt + 60^{\circ}.$ The contours are presented at intervals of 2 °K in beam temperature. The maps are given both in equatorial coordinates and, for the strip $-10^{\circ} \lt b^{11} \lt + 10^{\circ},$ in new Galactic coordinates.
ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/147.4.405