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5C 3.163 , the SIMBAD biblio (12 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST17:52:24 |
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. | |||||
1976MNRAS.177..137S | 94 | 11 | Observations of fine structure in very weak radio sources. | SPEED B. | |||||
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. | |||||
1980MNRAS.192..243U | 3 | 4 | 65 | Neutral hydrogen in the Andromeda nebula- II. H I emission in the north-east region of the nebula. | UNWIN S.C. | ||||
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 | 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. | |||||
1990ApJS...72..761B | 540 | 33 | The interstellar medium of M 31. II. A survey of 20 centimeter continuum emission. | BRAUN R. | |||||
2003A&A...398..937B | 13 | 36 | The polarized disk in M31 at λ6 cm. | BERKHUIJSEN E.M., BECK R. and HOERNES P. | |||||
2005ApJ...634..314T | 51 | 30 | XMM-Newton observations of the M31 northern disk: properties of selected X-ray sources and unresolved emission. | TRUDOLYUBOV S., KOTOV O., PRIEDHORSKY W., et al. | |||||
2021MNRAS.504.1801K | 44 | X | 1 | 10 | 7 | A lack of constraints on the cold opaque H I mass: H I spectra in M31 and M33 prefer multicomponent models over a single cold opaque component. | KOCH E.W., ROSOLOWSKY E.W., LEROY A.K., et al. |