223,633 research outputs found
No.407 Silvia Behrend
No full textTranscript (23 pages) of interview by Lorille Miller with Silvia Behrend on October 15, 1993Silvia Behrend (b. 1954) talks about her life, marriage, study for the ministry, and moving to Salt Lake City for the Unitarian Church with Lorille Miller
Siegfried Behrend
No full textCrítica del concierto del guitarrista alemán Siegfried Behrend, organizado por el Instituto Colombo Alemán. Interpretó obras de J. S.Bach, J. Haydn, N. Paganini, Fabritio Coroso, H. Villla Lobos, Manuel de Falla, Ambrosius y el propio Behrend.Medellín, Biblioteca Luis Echavarría Villegas, Sala de Patrimonio Documental, Archivo Luis Miguel de Zulateg
Heinrich Free: Die experimentelle Psychologie. Wiesbaden, Behrend 1896. 31 S.
No full textHEINRICH FREE: DIE EXPERIMENTELLE PSYCHOLOGIE. WIESBADEN, BEHREND 1896. 31 S.
Zeitschrift für Psychologie und Physiologie der Sinnesorgane (-)
Zeitschrift für Psychologie und Physiologie der Sinnesorgane (13) (a0004)
Heinrich Free: Die experimentelle Psychologie. Wiesbaden, Behrend 1896. 31 S. (13) (p0475
The gift [music] : song /
No full textH.179 (Publisher number). For voice and piano.; "No. 2 in E-flat".; Pl. no.: H.179.; Cover title.; "Dedicated to my friend Miss Erica Robertson".; "... composed expressly for Madam Antoinette Sterling".; Also available online http://nla.gov.au/nla.mus-an13416627
Crossing the bar [music] : song /
No full textH.851 (Publisher number). For voice and piano.; Cover title.; "No. 1 in D".; Pl. no.: H.851.; "Sung by Madam Antoinette Sterling".; Also available online http://nla.gov.au/nla.mus-an10320000; Library's copy in poor condition
A 2 h periodic variation in the low-mass X-ray binary Ser X-1
No full textSpectroscopy of the low-mass X-ray binary Ser X-1 using the Gran Telescopio Canarias have revealed a ?2 h periodic variability that is present in the three strongest emission lines. We tentatively interpret this variability as due to orbital motion, making it the first indication of the orbital period of Ser X-1. Together with the fact that the emission lines are remarkably narrow, but still resolved, we show that a main-sequence K dwarf together with a canonical 1.4 M? neutron star gives a good description of the system. In this scenario, the most likely place for the emission lines to arise is the accretion disc, instead of a localized region in the binary (such as the irradiated surface or the stream-impact point), and their narrowness is due instead to the low inclination (?10°) of Ser X-1
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