Hostname: page-component-848d4c4894-v5vhk Total loading time: 0 Render date: 2024-07-04T19:59:19.200Z Has data issue: false hasContentIssue false
  • English
  • Français

A High Resolution HI Survey of M31

Published online by Cambridge University Press:  04 August 2017

E. Brinks
E. Brinks*
Affiliation:
Leiden Observatory, Leiden, The Netherlands

Extract

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.

The first results of a new high resolution 21-cm HI line survey of M31 made with the Westerbork Synthesis Radio Telescope are presented. Five areas were mapped, covering the galaxy except for the extreme northern and southern parts, at a resolution of δα × δδ × δV = 24″ × 36″ × 3.2 km s−1. The spatial resolution corresponds to 30 × 120 pc at the distance of M31. This is of the same order as the resolution at the distance of the center or our own galaxy given by a 25-m dish. Consequently the M31 survey is comparable to surveys of the Milky Way galaxy in wealth of detail as well as in amount of data (∼ 1 Gigabyte).

Type
I. Kinematics of Gas and the Underlying Mass Distribution
Information
Symposium - International Astronomical Union , Volume 100: Internal Kinematics and Dynamics of Galaxies , 1983 , pp. 23 - 26
Copyright
Copyright © Reidel 1983 

References

Bajaja, E., Shane, W.W.: 1982, Astron. Astrophys. Suppl. Ser. 49, 745.Google Scholar
Cram, T.R., Roberts, M.S., Whitehurst, R.N.: 1980, Astron. Astrophys. Suppl. Ser. 40, 215.Google Scholar
Walterbos, R.A.M., Brinks, E., Shane, W.W.: in preparation.Google Scholar