48,562 research outputs found
[Letter from M. H. Westerman to Felix H. Morales- March 8, 1948]
No full textLetter sent by M. H. Westerman, City Secretary, to Felix H. Morales. Westerman advises Morales that the Baptist Mission has protested the granting of a liquor permit to the Cadillac Bar and Club. Westerman also informs Morales that he could appear before City Council in connection to the permit during the Council's regular meeting day
Interview with John Westerman
No full textAnn Pflaum interviews John Westerman, former general director of the University Hospitals and Clinics.Westerman, John H.; Pflaum, Ann M.. (1998). Interview with John Westerman. Retrieved from the University Digital Conservancy, https://hdl.handle.net/11299/48368
Liederen, voor Nederland.
No full textM.W. is M. Westerman ; H.J.R. is H.J. Rooseboom ; J.C.W. is J.C. WestermanEuropeana-GoogleBook
[Letter from John J. Herrera to M. H. Westerman - March 10, 1948]
No full textOnionskin carbon copy of a letter sent to M. H. Westerman, City Secretary at City Hall. Herrera advises that he his client, Felix H. Morales, would like to appear before City Council regarding the beer license for the Cadillac Bar
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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