31,806 research outputs found
Systems View of Coronavirus
No one envisioned the kinds of problems that emerged from the novel coronavirus nor had anyone considered its interactive scope. Now is the time to begin to redesign our processes and systems so that when confronted again we can cope and navigate better. Everyone needs to be a partner in these redesigns and each of the health, social, educational, and other systems must be integrated because it is their interconnections that coproduce and give meaning to our lives
No Open Cluster in the Ruprecht 93 Region
UBVI CCD photometry has been obtained for the Ruprecht 93 (Ru 93) region. We
were unable to confirm the existence of an intermediate-age open cluster in Ru
93 from the spatial distribution of blue stars. On the other hand, we found two
young star groups in the observed field: the nearer one (Ru 93 group) comprises
the field young stars in the Sgr-Car arm at d ~ 2.1 kpc, while the farther one
(WR 37 group) is the young stars around WR 37 at d ~ 4.8 kpc. We have derived
an abnormal extinction law (Rv = 3.5) in the Ruprecht 93 region.Comment: 6 pages, 6 figures, JKAS 2010, in press (Aug issue
UBVI CCD Photometry of the Open Cluster NGC 4609 and Hogg 15
UBVI CCD photometry is obtained for the open clusters NGC 4609 and Hogg 15 in
Crux. For NGC 4609, CCD data are presented for the first time. From new
photometry we derive the reddening, distance modulus and age of each cluster -
NGC 4609 : E(B-V) = 0.37 +/- 0.03, V_0 - M_V = 10.60 +/- 0.08, log tau = 7.7
+/- 0.1; Hogg 15 : E(B-V) = 1.13 +/- 0.11, V_0 - M_V = 12.50 +/- 0.15, log tau
<= 6.6. The young age of Hogg 15 strongly implies that WR 47 is a member of the
cluster. We have also determined the mass function of these clusters and have
obtained a normal slope (Gamma = -1.2 +/- 0.3) for NGC 4609 and a somewhat
shallow slope (Gamma = -0.95 +/- 0.5) for Hogg 15.Comment: 12 pages, 14 figures, JKAS, in pres
Linear Connections on Graphs
In recent years, discrete spaces such as graphs attract much attention as
models for physical spacetime or as models for testing the spirit of
non-commutative geometry. In this work, we construct the differential algebras
for graphs by extending the work of Dimakis et al and discuss linear
connections and curvatures on graphs. Especially, we calculate connections and
curvatures explicitly for the general nonzero torsion case. There is a metric,
but no metric-compatible connection in general except the complete symmetric
graph with two vertices.Comment: 22pages, Latex file, Some errors corrected, To appear in J. Math.
Phy
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