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The latest Rossiter-McLaughlin measurements of WASP systems David Brown (University of St Andrews) Et al Extreme Solar Systems 2; 13/9/2011

The latest Rossiter-McLaughlin measurements of WASP systems

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The latest Rossiter-McLaughlin measurements of WASP systems. David Brown (University of St Andrews) Et al. Extreme Solar Systems 2; 13/9/2011. Introduction. 18 Rossiter-McLaughlin measurements of WASP systems to date. Ongoing programs: HARPS for Southern targets - PowerPoint PPT Presentation

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Page 1: The latest Rossiter-McLaughlin measurements of WASP  systems

The latest Rossiter-McLaughlin measurements of WASP systems

David Brown(University of St Andrews)

Et al

Extreme Solar Systems 2; 13/9/2011

Page 2: The latest Rossiter-McLaughlin measurements of WASP  systems

Introduction•18 Rossiter-McLaughlin measurements of

WASP systems to date.•Ongoing programs:

▫HARPS for Southern targets▫SOPHIE for Northern targets

•Present 3 new WASP systems.▫Combined analysis of full photometric and

spectroscopic datasets.

Extreme Solar Systems 2; 13/9/2011

Page 3: The latest Rossiter-McLaughlin measurements of WASP  systems

WASP-16

Extreme Solar Systems 2; 13/9/2011

CORALIEHARPS

Page 4: The latest Rossiter-McLaughlin measurements of WASP  systems

WASP-16

Extreme Solar Systems 2; 13/9/2011

Brown et al (submitted)

CORALIEHARPSHARPS

Page 5: The latest Rossiter-McLaughlin measurements of WASP  systems

WASP-16•Circular orbit adopted.•No long-term trend detected.

•Teff = 5700 ± 150 K•λ = -4.6o +8.7

-10.0

•vsinI = 1.5 ± 0.5 km s-1

Extreme Solar Systems 2; 13/9/2011

Page 6: The latest Rossiter-McLaughlin measurements of WASP  systems

WASP-25

Extreme Solar Systems 2; 13/9/2011

Brown et al (submitted)

CORALIEHARPS

Page 7: The latest Rossiter-McLaughlin measurements of WASP  systems

WASP-25•Circular orbit adopted.•No long-term trend detected.

•Teff = 5750 ± 100 K•λ = 22.9o +8.9

-7.1

•vsinI = 3.2 ± 0.4 km s-1

Extreme Solar Systems 2; 13/9/2011

Page 8: The latest Rossiter-McLaughlin measurements of WASP  systems

WASP-31

Extreme Solar Systems 2; 13/9/2011

Brown et al (submitted)

CORALIEHARPS

Page 9: The latest Rossiter-McLaughlin measurements of WASP  systems

WASP-31•Circular orbit adopted.•No long-term trend detected.

•Teff = 6300 ± 100 K•λ = 1.6o ± 3.0•vsinI = 9.5 ± 1.1 km s-1

Extreme Solar Systems 2; 13/9/2011

Page 10: The latest Rossiter-McLaughlin measurements of WASP  systems

Integrating into the ensemble

Extreme Solar Systems 2; 13/9/2011

Brown et al (submitted)WASP-16

WASP-31WASP-25

Page 11: The latest Rossiter-McLaughlin measurements of WASP  systems

Integrating into the ensemble

Extreme Solar Systems 2; 13/9/2011

Brown et al (submitted)WASP-16

WASP-25WASP-31

Page 12: The latest Rossiter-McLaughlin measurements of WASP  systems

Integrating into the ensemble

Extreme Solar Systems 2; 13/9/2011

Brown et al (submitted)

See poster by Grant Miller (26.02)

WASP-16WASP-25WASP-31

Page 13: The latest Rossiter-McLaughlin measurements of WASP  systems

Integrating into the ensemble

Extreme Solar Systems 2; 13/9/2011

Brown et al (submitted)

Page 14: The latest Rossiter-McLaughlin measurements of WASP  systems

Integrating into the ensemble

Extreme Solar Systems 2; 13/9/2011

Brown et al (submitted)

Page 15: The latest Rossiter-McLaughlin measurements of WASP  systems

A new perspective?

Extreme Solar Systems 2; 13/9/2011

Triaud (submitted)

Page 16: The latest Rossiter-McLaughlin measurements of WASP  systems

A new perspective?

Extreme Solar Systems 2; 13/9/2011

Triaud (submitted)