Charm Physics at the Tevatron

First charm physics results from the CDF and D0 experiments at the Tevatron Run II are presented. With the addition of the Secondary Vertex Trigger CDF has become a competitive charm experiment.Comment: 4 pages, 11 figures proceedings of the XXXVIIIth Rencontres de Moriond on QCD and High Energy Hadronic Interactions, Les Arcs March 200

Woodbury, Town of and Woodbury Police Benevolent Association (Dispatchers)

In the Matter of TOWN OF WOODBURY, Orange County and WOODBURY POLICE BENEVOLENT ASSOCIATION (Dispatchers). FINDINGS OF FACT and RECOMMENDATIONS FOR RESOLUTION. Peter A. Korn, Fact Finder

Town of Eastchester and Eastchester White & Blue Collar Unit, CSEA Local 1000. AFSCME, AFL-CIO, Westchester County Local 860

In the matter of the fact-finding between the Town of Eastchester, employer, and the Eastchester White & Blue Collar Unit, CSEA Local 1000. AFSCME, AFL-CIO, Westchester County Local 860, union. PERB case no. M2011-041. Before: Peter A. Korn, fact finder

Croton-Harmon Union Free School District and Croton-Harmon Clerical Unit, CSEA, Local 860

In the matter of the fact-finding between the Croton-Harmon Union Free School District, employer, and the Croton-Harmon Clerical Unit, CSEA, Local 860, union. PERB case no. 2010-213. Before: Peter A. Korn, fact finder

Sleepy Hollow, Village of and Municipal Employee Unit, United Federation of Police Officers

In the matter of the fact-finding between the Village of Sleepy Hollow, employer, and the United Federation of Police Officers, Municipal Employee Unit, union. PERB case no. M2009-266. Before: Peter A. Korn, fact finder

Progress of analog-hybrid computation

Review of fast analog/hybrid computer systems, integrated operational amplifiers, electronic mode-control switches, digital attenuators, and packaging technique

Pristine CNO abundances from Magellanic Cloud B stars II. Fast rotators in the LMC cluster NGC 2004

We present spectroscopic abundance analyses of three main-sequence B stars in the young Large Magellanic Cloud cluster NGC 2004. All three targets have projected rotational velocities around 130 km/s. Techniques are presented that allow the derivation of stellar parameters and chemical abundances in spite of these high v sin i values. Together with previous analyses of stars in this cluster, we find no evidence among the main-sequence stars for effects due to rotational mixing up to v sin i around 130 km/s. Unless the equatorial rotational velocities are significantly larger than the v sin i values, this finding is probably in line with theoretical expectations. NGC 2004/B30, a star of uncertain evolutionary status located in the Blue Hertzsprung Gap, clearly shows signs of mixing in its atmosphere. To verify the effects due to rotational mixing will therefore require homogeneous analysis of statistically significant samples of low-metallicity main-sequence B stars over a wide range of rotational velocities.Comment: 12 pages, 5 figures, 2 tables; accepted for publication in ApJ (vol. 633, p. 899