Basic N-Body Modelling of the Evolution of Globular Clusters. I. Time
Scaling
Aarseth, S. J.
1998-05-28
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125 records were found.
Comment: Accepted for publication in MNRAS letters. 5 pages, 4 postscript
figures. Uses mn.cls. Also available at
http://panisse.lbl.gov/public/isobelpage/
Comment: 4 pages LaTeX, submitted to the "Eurokiel 2002: Galaxy Evolution III:
From Simple Models to Self Consistant Approaches" Conference Proceedings
Comment: To appear in Proc. of "Roentgenstrahlung from the Universe" held in
Wuerzburg, Germany, in Sept. 1995. 2 pages, 2 figures included, uuencoded
compressed Postscript
Comment: To appear in MNRAS. Latex file (10 pages of text) plus 14 separate
postscript figure files. Requires mn.sty. Postscript version with figures
embedded is available at http://www.ociw.edu/~lisa/publications.html
Comment: To appear in MNRAS. Latex file (4 pages of text) plus 3 separate
postscript figure files. Requires mn.sty. Postscript version with figures
embedded is available at http://www.ociw.edu/~lisa/publications.html
Comment: 52 LaTeX pages, 13 postscript figures, 3 tables, in AASTeX v4.0
format. To appear in ApJ, March 1, 1997, Vol. 477
Comment: 8 pages, 7 postscript figures, uses paspconf.sty and epsf.sty. To be
published in "The Young Universe: Galaxy Formation and Evolution at
Intermediate and High Redshift", 1998, S. D'Odorico, A. Fontana & E.
Giallongo (eds), (ASP). Also available at
http://panisse.lbl.gov/public/isobelpage/
Comment: Accepted for publication in MNRAS
The foreground component of the X-ray background can be studied by cross-correlating its intensity with galaxy catalogs. The two-point cross-correlation function between 67 Einstein X-ray fields and the APM galaxy catalogs was computed. A signal with an amplitude of W(sub xg) = 0.04 +/- 0.01, significant at the 3.5 sigma level, was computed. The reality of this signal was tested. The way in which this signal can be used to constrain models of the X-ray background is discussed.
Comment: 9 pages, 6 figures. Accepted for publication in MNRAS. Also available
from http://panisse.lbl.gov/public/isobelpage/ Corrected a few redshifts in
the tables, typos fixed, minor changes made to figures 4 and 5
