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Cluster & Association Cluster & Association Members Members Ernst Paunzen Ernst Paunzen IfA, Vienna IfA, Vienna

Cluster & Association Members

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Cluster & Association Members. Ernst Paunzen IfA, Vienna. Why consider Clusters Members?. Clusters offer astrophysical properties “for free”: Age Distance Reddening Not depending on any temperature, log g, absolute magnitude calibration. The BRITE HRD. - PowerPoint PPT Presentation

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Page 1: Cluster & Association  Members

Cluster & Association Cluster & Association MembersMembers

Ernst PaunzenErnst PaunzenIfA, ViennaIfA, Vienna

Page 2: Cluster & Association  Members

Why consider Clusters Why consider Clusters Members?Members?

Clusters offer astrophysical Clusters offer astrophysical properties “for free”:properties “for free”:

1.1. AgeAge

2.2. DistanceDistance

3.3. ReddeningReddening Not depending on any Not depending on any

temperature, log g, absolute temperature, log g, absolute magnitude calibrationmagnitude calibration

Page 3: Cluster & Association  Members

The BRITE HRDThe BRITE HRDWithout reddening: M(V) = -5 mag and V = 4 mag => distance = 630 pc

-6; 4; 1000-5; 4; 630-4; 4; 400-3; 4; 250-2; 4; 160-1; 4; 100+0; 4; 65

Page 4: Cluster & Association  Members

Clusters within 750 pcClusters within 750 pc-6; 4; 1000-5; 4; 630-4; 4; 400-3; 4; 250-2; 4; 160-1; 4; 100+0; 4; 65

log t < 8.0 (blue)log t < 9.0 (yellow)log t > 9.0 (red)

Several Cluster Members in the BRITE sample!

WEBDA: http://www.univie.ac.at/webda

Page 5: Cluster & Association  Members

Cluster Properties and Cluster Properties and MembershipMembership

Cluster formation within a few Cluster formation within a few MyrsMyrs

From one large Molecular CloudFrom one large Molecular Cloud Membership criteria due to proper Membership criteria due to proper

motions and radial velocitiesmotions and radial velocities

Page 6: Cluster & Association  Members

Isochrones IIsochrones I

Padova Isochrones

Page 7: Cluster & Association  Members

Isochrones IIIsochrones II

280KHuge Errors!

Page 8: Cluster & Association  Members

Lines of Equal MassesLines of Equal Masses

2.5

mag

Error:M(V) = 0.1 magMass = 0.1 M(sun)

+ Error in log Teff

Padova Isochrones

Page 9: Cluster & Association  Members

Precision of Age DeterminationPrecision of Age Determination

Values from the Literature Paunzen & Netopil, 2006, MNRAS, 371, 1641

Page 10: Cluster & Association  Members

Why consider Clusters Why consider Clusters Members?Members?

Clusters offer astrophysical Clusters offer astrophysical properties “for free”:properties “for free”:

1.1. Age, error about 15%Age, error about 15%2.2. Distance, error less than 10%Distance, error less than 10%3.3. Reddening, error less than 5%Reddening, error less than 5%

Values can be improved!Values can be improved! ““Only positive membership Only positive membership

needed” needed” Precise mass estimation possiblePrecise mass estimation possible Huge data base (WEBDA) in ViennaHuge data base (WEBDA) in Vienna