WSTB 37W91 , the SIMBAD biblio

WSTB 37W91 , the SIMBAD biblio (13 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST07:00:06

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
1969MNRAS.144..101P 217 137 5C3 : a radio continuum survey of M 31 and its neighbourhood. POOLEY G.G.
1974A&A....34..173B 91 38 A radio continuum survey of M 31 at 2695 MHz. BERKHUIJSEN E.M. and WIELEBINSKI R.
1977A&A....57....9B 22 64 A radio continuum survey of M 31 at 2695 MHz. II. Comparison of radio and optical data. BERKHUIJSEN E.M.
1983A&A...117..141B 65 24 A radio continuum survey of M 31 at 4850 MHz. BERKHUIJSEN E.M., WIELEBINSKI R. and BECK R.
1984A&AS...56..245B 409 21 A high resolution radio continuum survey of Messier 31. I. Observations at 610 MHz, data reduction, and the 36W catalogue of radio sources. BYSTEDT J.E.V., BRINKS E., DE BRUYN A.G., et al.
1985A&AS...61..451W viz 256 36 A high resolution radio continuum survey of Messier 31. II. Observations at 1412 MHz, data reduction and the 37W catalogue of radio sources. WALTERBOS R.A.M., BRINKS E. and SHANE W.W.
1989A&A...222...58B 1 9 51 High-resolution polarization observations of M 31. I. Structure of the magnetic field in the southwestern arm. BECK R., LOISEAU N., HUMMEL E., et al.
1990ApJS...72..761B 540 33 The interstellar medium of M 31. II. A survey of 20 centimeter continuum emission. BRAUN R.
1993ApJ...405..153D 23 27 An HI absorption survey of M 31 and M 33 : the mixture ofwarm and cool phases in the interstellar media of spiral galaxies. DICKEY J.M. and BRINKS E.
1998A&A...335.1117H 36 68 New clues to the magnetic field structure of M 31. HAN J.L., BECK R. and BERKHUIJSEN E.M.
1998A&AS..129..329B 40 27 A deep λ20 cm radio continuum survey of M 31. BECK R., BERKHUIJSEN E.M. and HOERNES P.
2003A&A...398..937B 13 36 The polarized disk in M31 at λ6 cm. BERKHUIJSEN E.M., BECK R. and HOERNES P.
2004NewAR..48.1289B 29 46 Observations of magnetic fields in the Milky Way and in nearby galaxies with a Square Kilometre Array. BECK R. and GAENSLER B.M.

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