1969
DOI: 10.1111/j.1467-9248.1969.tb00745.x
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The Political Strength of British Agriculture

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Cited by 4 publications
(3 citation statements)
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“…One obvious advantage of such an approach is connected with the time scales of various accretion phenomena, which are sufficiently short, so as to avoid any major observational bias: the mass accretion rates in CVs, as we already said, range from ∼10 −11 to 10 −8 M yr −1 ; the time scales are from tens of seconds (oscillations in dwarf novae at outbursts) to years (for example, the super-outbursts of SU UMa stars or the long-term variations in VY Scl stars). SS Cygni shows oscillations of ∼10 s both in optical and in X-ray ranges, orbital modulations (P orb 6.6 h) of the intensities of Balmer and UV emission lines and of the continuum, and almost periodic outbursts (P outb ∼ 50 days, Howarth 1978). All these characteristics together with the relative high luminosity both in outburst and in quiescence render SS Cygni the most appropriate laboratory for studying the physical processes occurring in dwarf novae and in CVs in general (see the review by Giovannelli & Martinez-Pais 1991).…”
Section: Introductionmentioning
confidence: 99%
“…One obvious advantage of such an approach is connected with the time scales of various accretion phenomena, which are sufficiently short, so as to avoid any major observational bias: the mass accretion rates in CVs, as we already said, range from ∼10 −11 to 10 −8 M yr −1 ; the time scales are from tens of seconds (oscillations in dwarf novae at outbursts) to years (for example, the super-outbursts of SU UMa stars or the long-term variations in VY Scl stars). SS Cygni shows oscillations of ∼10 s both in optical and in X-ray ranges, orbital modulations (P orb 6.6 h) of the intensities of Balmer and UV emission lines and of the continuum, and almost periodic outbursts (P outb ∼ 50 days, Howarth 1978). All these characteristics together with the relative high luminosity both in outburst and in quiescence render SS Cygni the most appropriate laboratory for studying the physical processes occurring in dwarf novae and in CVs in general (see the review by Giovannelli & Martinez-Pais 1991).…”
Section: Introductionmentioning
confidence: 99%
“…It seemed, indeed, that in the early post-war decades an electoral market was emerging for the farm vote. What particularly worried economic commentators, though, was that the favours politicians were granting were leading to excessive subsidies and market distortions (Gardener, 1979;Howarth, 1969). Economists, as well as some political scientists, therefore, who considered such a response economically irrational sought to scrutinise its political rationality.…”
Section: The Farming Votementioning
confidence: 99%
“…Economists, as well as some political scientists, therefore, who considered such a response economically irrational sought to scrutinise its political rationality. And to do so, they set out to establish the size of the farm vote (Self and Storing, 1962;Howarth, 1969;Benyon and Harrison, 1962;Pennock, 1959). Although there were differences in methodology a number of overlapping points emerged.…”
Section: The Farming Votementioning
confidence: 99%