Changes between Version 1 and Version 2 of GravoTurbulence

Timestamp:

05/17/11 12:58:23 (14 years ago)

Author:

Jonathan

Comment:

—

GravoTurbulence

@@ -28 +28 @@
 * [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008AJ....136..404O&db_key=AST&link_type=ABSTRACT&high=4dd2954bad03054 Offner et al. 2008]
 * [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ApJ...727L..20K&db_key=AST&link_type=ABSTRACT&high=4dd2954bad03054 Kritsuk et al 2011]
+ * ENZO 512^3^+5x2=524,288^3^; 5pc -> 2 AU; Isothermal 10K; n=500/cc
+ * Power law tail to density pdf
 * [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ApJ...693..914O&db_key=AST&link_type=ABSTRACT&high=4dd2954bad03054 Offner et al 2009]
 * [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011MNRAS.410L...8C&db_key=AST&link_type=ABSTRACT Cho & Kim 2011]
+ * 512^3^ Isothermal MHD fixed grid
+ * beta=.1
+ * J=4 (l_box/l_jeans)
+ * M=10
+ * Power law tail
+ * Line-width size relation
 * [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ApJ...731...59C&db_key=AST&link_type=ABSTRACT Collins et al 2011]
+ * ENZO 128^3^+4 = 2048^3^; 10pc -> 1000 AU; MHD Isothermal 10K; n=300/cc; B=.6+-2.7 microG (no AD) (supercritical)
+ * power law tail for density (1.64) and B (2.74)
+ * B = rho^.48^
+ * sigma = rho^.25^ for cores
+ * CMF = 2.1+-.6
+* [http://adsabs.harvard.edu/abs/2008ApJ...687..354N Nakamura & Li 2008]
+ * 128^3^ isothermal MHD with AD and feedback 2.4 pc -> .02 pc
+ * B=15 microG (beta=1/24) subcritical
+* [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ApJ...684..395H&db_key=AST&link_type=ABSTRACT&high=4dd2954bad01462 Hennebelle & Chabrier 2008]