Search Results - (Author, Cooperation:G. C. Clayton)
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1M. Matsuura ; E. Dwek ; M. Meixner ; M. Otsuka ; B. Babler ; M. J. Barlow ; J. Roman-Duval ; C. Engelbracht ; K. Sandstrom ; M. Lakicevic ; J. T. van Loon ; G. Sonneborn ; G. C. Clayton ; K. S. Long ; P. Lundqvist ; T. Nozawa ; K. D. Gordon ; S. Hony ; P. Panuzzo ; K. Okumura ; K. A. Misselt ; E. Montiel ; M. Sauvage
American Association for the Advancement of Science (AAAS)
Published 2011Staff ViewPublication Date: 2011-07-09Publisher: American Association for the Advancement of Science (AAAS)Print ISSN: 0036-8075Electronic ISSN: 1095-9203Topics: BiologyChemistry and PharmacologyComputer ScienceMedicineNatural Sciences in GeneralPhysicsPublished by: -
2Schulte-Ladbeck, R. E. ; Clayton, G. C. ; Leitherer, C. ; Drissen, L. ; Robert, C. ; Nota, A. ; Parker, J. WM.
Springer
Published 1993Staff ViewISSN: 1572-9672Keywords: Luminous Blue Variables ; B [e] stars ; polarizationSource: Springer Online Journal Archives 1860-2000Topics: PhysicsNotes: Abstract We are in the process of surveying the linear polarization in luminous, early-type stars. We here report on new observations of the B [e] stars S 18 and R 50, and of the Luminous Blue Variables HR Car, R 143, and HD 160529. Together with previously published data, these observations provide clear evidence for the presence of intrinsic polarization in 1 B[e] star (HD 34664) and in 5 LBVs (ν Car, P Cyg, R 127, AG Car, and HR Car). The data indicate that anisotropic stellar winds are a common occurrence among massive stars in these particular evolutionary stages. For such stars, mass-loss rates estimated using the assumption of a spherical, homogeneous and stationary outflow may be in error.Type of Medium: Electronic ResourceURL: -
3Staff View
ISSN: 0365-9496Keywords: Chemistry ; Inorganic ChemistrySource: Wiley InterScience Backfile Collection 1832-2000Topics: Chemistry and PharmacologyType of Medium: Electronic ResourceURL: