use Boomshakalaka\StellarWP\Assets\Asset; Asset::add( 'my-asset', 'css/some-asset.css', $an_optional_version, $an_optional_path_to_project_root ) ->add_style_data( 'rtl', true ) ->add_style_data( 'suffix', '.rtl' ) ->add_to_group( 'my-assets' ) // You can have more th...
We also present the time evolution of ejection rates forgas and metals for two different {\\bf I}nitial {\\bf M}ass {\\bf F}unctions ({\\bfIMF}s) as well as cosmological and evolutionary corrections for all the filtersas a function of redshift and two different cosmologies. ...
转格式 31阅读文档大小:89.77K5页yzhlyb上传于2015-05-29格式:PDF measuring the accreting stellar and intermediate mass black hole populations in the galaxy and local group 热度: 【30页精品】A FUSE Survey of Interstellar Molecular Hydrogen in the Small and Large Magellanic Clouds ...
distributions.Itisfoundthatthemass-to-lightratiosasderivedfromajointlens- ingandstellardynamicsanalysisarevirtuallyconsistentwiththoseobtainedfrom theuseoftheFundamentalPlane.Also,forHST14113+5211,wefindthatthetotal massdistributioniswellreproducedbyapower-lawdensityprofilewithanindexof ...
ies we may conclude that dSphs in the Local Group do not have a significant number of bright X-ray sources (see Zang & Meurs 2001). The number of binary X-ray sources in a galaxy is determined by the formation rate of the sources and the ...