168 research outputs found
A Chandra X-ray Study of the Globular Cluster M80
We report our analysis of a Chandra X-ray observation of the rich globular
cluster M80, in which we detect some 19 sources to a limiting 0.5-2.5 keV X-ray
luminosity of 7*10^30 ergs/s within the half-mass radius. X-ray spectra
indicate that two of these sources are quiescent low-mass X-ray binaries
(qLMXBs) containing neutron stars. We identify five sources as probable
cataclysmic variables (CVs), one of which seems to be heavily absorbed,
implying high inclination. The brightest CV may be the X-ray counterpart of
Nova 1860 T Sco. The concentration of the X-ray sources within the cluster core
implies an average mass of 1.2+/-0.2 Msun, consistent with the binary nature of
these systems and very similar to the radial distribution of the blue
stragglers in this cluster. The X-ray and blue straggler source populations in
M80 are compared to those in the similar globular cluster 47 Tuc.Comment: Submitted to ApJ. 15 pages, 6 figure
The Measurement of Solar Diameter and Limb Darkening Function with the Eclipse Observations
The Total Solar Irradiance varies over a solar cycle of 11 years and maybe
over cycles with longer period. Is the solar diameter variable over time too?
We introduce a new method to perform high resolution astrometry of the solar
diameter from the ground, through the observations of eclipses by reconsidering
the definition of the solar edge. A discussion of the solar diameter and its
variations must be linked to the Limb Darkening Function (LDF) using the
luminosity evolution of a Baily's Bead and the profile of the lunar limb
available from satellite data. This approach unifies the definition of solar
edge with LDF inflection point for eclipses and drift-scan or heliometric
methods. The method proposed is applied for the videos of the eclipse in 15
January 2010 recorded in Uganda and in India. The result shows light at least
0.85 arcsec beyond the inflection point, and this suggests to reconsider the
evaluations of the historical eclipses made with naked eye.Comment: 16 pages, 11 figures, accepted in Solar Physics. arXiv admin note:
text overlap with arXiv:astro-ph/0601109 by other author
Über den Einfluß der Korngröße auf die Remanenz von weichem Eisen und über den Einfluß der Scherung auf die Bestimmung der wahren Remanenz
Studien in der Bernsteinsäure- und Glutarsäure-Gruppe. Ueber Anilsäuren und Anile alkylirter Bernsteinsäuren und Glutarsäuren
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De stad in de schijnwerpers. Stadsgeschiedenis in Belgische en Nederlandse historische tijdschriften (2013)
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Rearrangement of 5-aryl-1,1-dichloro-5-hydroxy- and 5-aryl-1,1,5-trichloro-1,3-pentadienes into 5-aryl-2.4-pentadienoic acids
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