Zobrazeno 1 - 10
of 127
pro vyhledávání: '"L. A. Whitehouse"'
Publikováno v:
Diagnostic Histopathology. 26:233-236
Primary lymphoma of the thyroid is an uncommon malignancy, whereas papillary thyroid carcinoma is the most common thyroid malignancy. Both have an association with Hashimoto's thyroiditis. We discuss a case of an 83 year old male who presented with a
Autor:
Fatima Nadat, Chris F. Inglehearn, Laura Wilkinson Hewitt, Alan J. Mighell, Claire E. L. Smith, Helen D. Rodd, James A. Poulter, Laura L. E. Whitehouse, Thomas A. Edwards, Brian R. Jackson, Iain W. Manfield
Publikováno v:
Human Molecular Genetics
Amelogenesis is the process of enamel formation. For amelogenesis to proceed, the cells of the inner enamel epithelium (IEE) must first proliferate and then differentiate into the enamel-producing ameloblasts. Amelogenesis imperfecta (AI) is a hetero
Publikováno v:
Atmospheric Chemistry and Physics, Vol 4, Iss 7, Pp 2057-2081 (2004)
This paper presents a formal method of species lumping that can be applied automatically to intermediate compounds within detailed and complex tropospheric chemical reaction schemes. The method is based on grouping species with reference to their che
Externí odkaz:
https://doaj.org/article/118e698f146a449396555448c6723b11
Publikováno v:
Atmospheric Chemistry and Physics, Vol 4, Iss 7, Pp 2025-2056 (2004)
Explicit mechanisms describing the complex degradation pathways of atmospheric volatile organic compounds (VOCs) are important, since they allow the study of the contribution of individual VOCS to secondary pollutant formation. They are computational
Externí odkaz:
https://doaj.org/article/ba079fe437654f4b9b23626fac10ee46
Autor:
Andrew Swan, J Guo, Nikolay Walters, Thomas G. Wilson, I. D. Howarth, Jay Farihi, S. Mancino, L J Whitehouse
Many characteristics of dwarf carbon stars are broadly consistent with a binary origin, including mass transfer from an evolved companion. While the population overall appears to have old-disc or halo kinematics, roughly 2$\,$per cent of these stars
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b80928970111877284a1dccf5f132249
http://arxiv.org/abs/2105.00036
http://arxiv.org/abs/2105.00036
Autor:
Caroline Brown, Claire E. L. Smith, Rowena E. Mitchell, Elizabeth O’Sullivan, Laura L. E. Whitehouse, Lucy Brown, Ian R. Berry, Chris F. Inglehearn, Teresa Lamb, Alan J. Mighell, James A. Poulter, Ruth Charlton, Anup Patel
Publikováno v:
Oral Diseases
Objectives: Variants in DLX3 cause tricho‐dento‐osseous syndrome (TDO, MIM #190320), a systemic condition with hair, nail and bony changes, taurodontism and amelogenesis imperfecta (AI), inherited in an autosomal dominant fashion. Different varia
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 477:3801-3806
This paper reports preliminary yet compelling kinematical inferences for N ~ 600 carbon-rich dwarf stars that demonstrate around 30% to 60% are members of the Galactic halo. The study uses a spectroscopically and non-kinematically selected sample of
Autor:
Alan J. Mighell, Teresa Lamb, Rowena E. Mitchell, Anup Patel, Elizabeth O’Sullivan, Chris F. Inglehearn, James A. Poulter, Caroline Brown, Lucy Brown, Claire E. L. Smith, Ian R. Berry, Ruth Charlton, Laura L. E. Whitehouse
Publikováno v:
Oral Surgery, Oral Medicine, Oral Pathology and Oral Radiology. 132:e52
Background Variants in DLX3 cause tricho-dento-osseous syndrome (TDO; MIM accession no. 190320), a systemic condition with hair, nail, and bony changes, taurodontism, and amelogenesis imperfecta (AI) inherited in an autosomal dominant fashion. Differ
Autor:
L. Barber, Harold L. K. Whitehouse
Publikováno v:
EDULEARN Proceedings.
Dwarf carbon stars make up the largest fraction of carbon stars in the Galaxy with around 1200 candidates known to date primarily from the Sloan Digital Sky Survey. They either possess primordial carbon-enhancements, or are polluted by mass transfer
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::302bed78758bbc8f5824b429d32dd2f9
http://arxiv.org/abs/1806.06074
http://arxiv.org/abs/1806.06074