Titlebook: Unmarried Motherhood in the Metropolis, 1700–1850; Pregnancy, the Poor Samantha Williams Book 2018 The Editor(s) (if applicable) and The A

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The Workhouse,itable lying-in hospitals. In this chapter Williams provides the first systematic assessment of the role of the workhouse for unmarried mothers. Evidence is presented on the proportion of women who gave birth in the workhouse and the time that they spent there. The workhouse of St. Martin in the Fie

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Maintenance,re identified and affiliated in the magistrates’ court. However, the amount recovered by fathers was very low in London; this was a failing system. More detailed evidence on the occupations of putative fathers than has been explored by historians hitherto shows that fathers were not necessarily repr

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Punishment,ity and maintenance payments, as well as to the church courts for fornication. This chapter charts trends in commitments to the London houses of correction for bastardy. There was a division by gender, with women being committed to Bridewell and men to Clerkenwell and Tothill Fields. The most remark

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Conclusions, poor law, sexuality and illegitimacy were ‘mutually constitutive’. There was a distinctly metropolitan flavour to both courtship and to welfare. The chapter reflects upon the varied experiences of unmarried mothers and of conflicting evidence. The Poor Law Amendment Act of 1834 was a watershed in p

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Book 2018elief expenditure. In doing so, she explores the experience of being an unmarried mother from courtship and conception, through the discovery of pregnancy, and the birth of the child in lodgings or one of the new parish workhouses. Although fathers were generally held to be financially responsible f

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in der Presse oder in den explizit als ?Kultur“ im Rundfunk ausgewiesenen Sendungen thematisiert wird. Kulturelle Belange und Auseinandersetzungen k?nnen und werden durchaus im Politikteil, aber auch im Wirtschaftsteil und speziell auch im Lokalteil der Presse thematisiert, handle es nun um radikal

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Samantha Williamstwo different days. (This certainly poses some problems with respect to changing seeing quality and instrument stability)..After correcting the E-W data for solar rotation two-dimensional FFT transforms were performed in order to compare the power in the two sets of data as a function of . and l. Th

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