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Variable Blue Stragglers in M67 Zhang Xiao-Bin NAOC

Variable Blue Stragglers in M67

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Variable Blue Stragglers in M67. Zhang Xiao-Bin NAOC. Abstract. - PowerPoint PPT Presentation

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Page 1: Variable Blue Stragglers in M67

Variable Blue Stragglers in M67

Zhang Xiao-Bin NAOC

Page 2: Variable Blue Stragglers in M67

Abstract A long-term time-series CCD photometry on variabl

e 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.

Page 3: Variable Blue Stragglers in M67

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 under-loop 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;

Page 4: Variable Blue Stragglers in M67

All relying on the complete understanding of the properties and evolutionary status of BSs;

Variable BSs (photometric and/or spectroscopic): the most ideal samples;

Page 5: Variable Blue Stragglers in M67

BSs in M67 M67: with the age similar to the Sun; extensively ob

served; More than 30 BSs identified; More than 10 BSs are proved to be photometric an

d/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;

Page 6: Variable Blue Stragglers in M67
Page 7: Variable Blue Stragglers in M67

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.

Page 8: Variable Blue Stragglers in M67

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

Page 9: Variable Blue Stragglers in M67

Light curve analysis: Physical parameters:

adopting the distance modulus

of the cluster

Page 10: Variable Blue Stragglers in M67

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…