* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project
Download Variable Blue Stragglers in M67
		                    
		                    
								Survey							
                            
		                
		                
                            
                            
								Document related concepts							
                        
                        
                    
						
						
							Transcript						
					
					Variable Blue Stragglers in M67 Zhang Xiao-Bin NAOC Abstract  A long-term time-series CCD photometry on variable blue stragglers (BSs) was performed, aiming on the understanding of the properties and physical nature of the BSs based on the comprehensive photometric study. I report here the progress and some results drawn from this project. Blue stragglers    Bluer and brighter than the turn-off of the stellar population; noticed first by Sandage (1953) in the GC M3; BSs related: yellow or red stragglers; up and underloop stars; Origin: complicated proceedings; many theories:      Binary merger; Multiple epochs of star formation; Star-life extend due to internal mixing; Mass-transfer within binary stars; Stellar collisions;   All relying on the complete understanding of the properties and evolutionary status of BSs; Variable BSs (photometric and/or spectroscopic): the most ideal samples; BSs in M67     M67: with the age similar to the Sun; extensively observed; More than 30 BSs identified; More than 10 BSs are proved to be photometric and/or spectroscopic variables; Well-classified photometric variable BSs:  1 RS CVn star: S1082;  2 W Uma systems: S1036 and S1282;  2 oscillation BSs: S1280 and S1284; The long-term photometry   BATC: Feb. 2001; 85 cm reflector:     Dec. 2003 – Jan. 2004; Dec. 2004 – Jan. 2004; Complete photometric study has been finished for S1282, S1280 and S1284; physical parameters for the 3 variable BSs are determined, evolutionary status and probable formation mechanism are discussed; S1036 and S1082; waiting for more observations. S1282, an example  W Uma system discovered early in 1960; orbital and physical parameters are very uncertain; almost at the turn-off in the CMD   Light curve analysis: Physical parameters: adopting the distance modulus of the cluster  Discussions:     The primary: un-evolved normal MS star; the deduced mass matches its position in the CMD (the turn-off mass of M67: 1.25 solar mass); The secondary: over-radius, over-luminosity, obviously evolved; Mass transfer and mass ratio inverse undergone; To be a BS…