Zobrazeno 1 - 10
of 21
pro vyhledávání: '"Graham Berriman"'
Publikováno v:
The Astrophysical Journal Supplement Series. 104:117
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ee59cf617fc3a989da2c1f2359a923e2
https://doi.org/10.1086/192295
https://doi.org/10.1086/192295
Autor:
Gary D. Schmidt, Dayal Wickramasinghe, Graham Berriman, H. S. Stockman, James Liebert, R. L. Moore
Publikováno v:
The Astrophysical Journal. 401:628
The AM Her-type of mass-transfer binary displays strong circular polarization in its optical flux, due to high harmonic cyclotron emission from the vicinity of the accretion shock. Circular polarization is the best direct evidence for magnetic white
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0523fa7e642603a19a356dbe2664346f
https://doi.org/10.1086/172091
https://doi.org/10.1086/172091
Publikováno v:
Scopus-Elsevier
Effective temperatures have been recalculated for the M dwarf observed by Berriman and Reid in 1987 (MNRAS, 227), using updated apparent magnitudes where appropriate. The results show that the corrections to the photometry have little effect on the d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1870630782a0dc6231e9dee8c52d8499
https://doi.org/10.1086/186418
https://doi.org/10.1086/186418
Publikováno v:
The Astrophysical Journal Supplement Series. 74:869
Les observations polarimetriques optiques d'un ensemble, complet jusqu'a la magnitude B = 16.2, de 114 quasars du Palomar-Green Bright Quasar Survey sont presentees. La distribution et la variabilite de la polarisation sont analysees.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4625267ee839a04ab2c36a840f4b57b4
https://doi.org/10.1086/191523
https://doi.org/10.1086/191523
Autor:
Graham Berriman
Publikováno v:
The Astrophysical Journal. 354:148
This paper uses the variation with redshift of the near-infrared colors of the Palomar Green Bright Quasars as the basis for an analysis of the origin of their infrared light. Comparison of the data with simple models of the continuum, appropriately
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d4d1acf560afd7e663bf462a4790eb5d
https://doi.org/10.1086/168674
https://doi.org/10.1086/168674
Autor:
Klaus Reinsch, Jeremy Bailey, P. A. Charles, Tim Naylor, B. Warner, Graham Berriman, G. T. Bath, B. J. M. Hassall
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 229:183-202
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e8a3ff8177f81418150c7ac800f630ca
https://doi.org/10.1093/mnras/229.2.183
https://doi.org/10.1093/mnras/229.2.183
Autor:
Graham Berriman
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 228:729-743
Premiere analyse detaillee des formes des eclipses IR de cette nova naine, composee d'une naine blanche au centre d'un disque d'accretion avec une tache lumineuse a sa crete, et d'un compagnon naine rouge
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3306cf2d434e18f0e92dc7f1a294a295
https://doi.org/10.1093/mnras/228.3.729
https://doi.org/10.1093/mnras/228.3.729
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 217:327-346
Origine de la lumiere IR entre 1 et 2 μm pour un echantillon de 28 binaires cataclysmiques, pour la plupart des novae naines en repos. La lumiere IR provient de la naine rouge qui fournit de la matiere a son compagnon naine blanche et au disque d'ac
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::44947755c35ecd47101a6f668540e079
https://doi.org/10.1093/mnras/217.2.327
https://doi.org/10.1093/mnras/217.2.327
Autor:
Frank M. Bateson, I. M. Coulson, Brian Warner, P. A. Charles, Graham Berriman, K. Reinsch, Patricia A. Whitelock, Jeremy Bailey, Tim Naylor, A. R. Hyland
Publikováno v:
International Astronomical Union Colloquium. 93:365-369
We present optical and IR observations of the dwarf nova OY Car during the May 1985 superoutburst. From them we find that the superhump has a temperature of ~8000K and an area of order half the size of the red dwarf or accretion disk. We also compare
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::73f49d429368ac12e9ce6740b69ce741
https://doi.org/10.1017/s0252921100105093
https://doi.org/10.1017/s0252921100105093
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 219:629-655
Photometrie en lumiere blanche a haute vitesse de cette variable cataclysmique, afin d'etudier la structure du systeme et de deriver les proprietes de ses composantes
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d4e49e522e161e88a261fb7aaef0f5ea
https://doi.org/10.1093/mnras/219.3.629
https://doi.org/10.1093/mnras/219.3.629