Changes between Version 10 and Version 11 of GravoTurbulence

Timestamp:

07/01/11 11:24:33 (14 years ago)

Author:

Jonathan

Comment:

—

GravoTurbulence

@@ -82 +82 @@
 * [http://adsabs.harvard.edu/abs/2009ApJ...702.1428H Hennebelle & Chabrier 2009] Analytical Theory for the Initial Mass Function. II. Properties of the Flow
 * [http://adsabs.harvard.edu/abs/2011arXiv1101.4940H Hopkins et al 2011] Self-Regulated Star Formation in Galaxies via Momentum Input from Massive Stars
-* [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ApJ...699.1092H&db_key=AST&link_type=ABSTRACT&high=4dd2954bad03054 Heyer et al. 2009]
+* [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ApJ...699.1092H&db_key=AST&link_type=ABSTRACT&high=4dd2954bad03054 Heyer et al. 2009] Re-Examining Larson's Scaling Relationships in Galactic Molecular Clouds
 * [http://adsabs.harvard.edu/abs/1986ApJ...305..309H Hunter et al 1986] Star formation in colliding gas flows
 * [http://adsabs.harvard.edu/abs/2005A%26A...435..611J Jappsen et al 2005] The stellar mass spectrum from non-isothermal gravoturbulent fragmentation
@@ -113 +113 @@
 * [http://adsabs.harvard.edu/abs/1976ApJ...210..326M Mouschovias & Spitzer 1976] Note on the collapse of magnetic interstellar clouds
 * [http://adsabs.harvard.edu/abs/1991ApJ...373..169M Mouschovias 1991] Magnetic braking, ambipolar diffusion, cloud cores, and star formation - Natural length scales and protostellar masses
-* [http://adsabs.harvard.edu/abs/2008ApJ...687..354N Nakamura & Li 2008]
+* [http://adsabs.harvard.edu/abs/2008ApJ...687..354N Nakamura & Li 2008] Magnetically Regulated Star Formation in Three Dimensions: The Case of the Taurus Molecular Cloud Complex
  * 128^3^ isothermal MHD with AD and feedback 2.4 pc -> .02 pc
  * B=15 microG (beta=1/24) subcritical