introduction to binary stars steve b. howell noao

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Introduction to Introduction to Binary Stars Binary Stars Steve B. Howell NOAO

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Page 1: Introduction to Binary Stars Steve B. Howell NOAO

Introduction to Binary StarsIntroduction to Binary Stars

Steve B. Howell

NOAO

Page 2: Introduction to Binary Stars Steve B. Howell NOAO

Binary Stars ??Binary Stars ??

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Page 3: Introduction to Binary Stars Steve B. Howell NOAO

Binary Stars ??Binary Stars ??

0 1

Page 4: Introduction to Binary Stars Steve B. Howell NOAO

Binary Stars - Binary Stars -

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Binary stars are pairs of stars orbiting each other “connected’ by their mutual gravitational interaction.

50% of stars are binaries: ~100% O/B ~75% M Obs. biases

Page 5: Introduction to Binary Stars Steve B. Howell NOAO

Binary Stars - Binary Stars -

Binary Stars may have orbital periods from seconds to hours to thousands of years

They may contain stars of all kinds, sizes, and masses

They may have circular or elliptical orbits They are believed to have formed together -

same age (not capture) Close binaries affect each other’s evolution Long period binaries essentially act as single

stars

Page 6: Introduction to Binary Stars Steve B. Howell NOAO

Binary Stars - TypesBinary Stars - Types

Binary stars come in a few types differentiated by their orbital period and/or observational behavior. For example:– Visual double (actually see both

components - LONG period). Do not confuse with optical double

– Astrometric binaries - see the wobble on the sky

Page 7: Introduction to Binary Stars Steve B. Howell NOAO

Binary Stars - TypesBinary Stars - Types

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An astrometric and visual binary: Sirius A&B -- an A star (A) and a white dwarf (B)

Has a ~50 year orbit. 8.6 light years from Earth

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Chandra Image

Page 8: Introduction to Binary Stars Steve B. Howell NOAO

Binary Stars - TypesBinary Stars - Types

or– Eclipsing binaries - one/two eclipses per

orbit – Spectrum binaries - spectral properties

change– Spectroscopic binaries - radial velocity

motions (short periods easier to find)

Page 9: Introduction to Binary Stars Steve B. Howell NOAO

Binary Stars - TypesBinary Stars - Types

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Schematic and real eclipsing binary light curves

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Page 10: Introduction to Binary Stars Steve B. Howell NOAO

Binary Stars - TypesBinary Stars - Types

Spectral variations over time due to the binary nature of this star

Page 11: Introduction to Binary Stars Steve B. Howell NOAO

Binary Stars - TypesBinary Stars - Types

Or differentiated by other criteria- – Close binaries w/ stellar distortions or

mass transfer – Intrinsic brightness changes due to stellar

variability– Binaries with components of very different

properties: color (WD+RD), mass (Exo-Planet), temperature

– Other

Page 12: Introduction to Binary Stars Steve B. Howell NOAO

Binary Stars - Types Binary Stars - Types

Binaries can be close (short orbital period) and show light variations due to …

Ellipsoidal shape and/or tidal interaction

Interactions such as mass exchange / transfer

If the smaller (but more massive) star in an IB is a white dwarf, the binary is called a cataclysmic variable

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Page 13: Introduction to Binary Stars Steve B. Howell NOAO

Binary Stars - TypesBinary Stars - Types

All combinations of the previous properties are possible

Many are unknown as they simply have not been seen to vary (line of sight / observed)

Binary Stars are the fundamental way in which we understand stars (and star systems): their formation, evolution & death.

Remember --Three out of every two stars are in a binary system

Page 14: Introduction to Binary Stars Steve B. Howell NOAO

Binary Stars - What can we learn?Binary Stars - What can we learn?

Eclipsing binaries are the best as the light curve can give stellar masses, radii, temperatures,& age estimates

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Page 15: Introduction to Binary Stars Steve B. Howell NOAO

Binary Stars - What can we learn?Binary Stars - What can we learn? Eclipsing (or not) Radial velocity curve

can give masses (or mass estimate)

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RV amplitudes give K1 & K2

Page 16: Introduction to Binary Stars Steve B. Howell NOAO

Binary Stars - What can we learn?Binary Stars - What can we learn? For a circular orbit

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Measure semi-major axis, a, from projected orbit & the distance.Relative positions about the center give: M1/M2 = a2/a1 = K2/K1

Kepler’s Law

Page 17: Introduction to Binary Stars Steve B. Howell NOAO

Mass vs. radius and luminosityMass vs. radius and luminosity

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Page 18: Introduction to Binary Stars Steve B. Howell NOAO

The Oddest Eclipsing Binary?The Oddest Eclipsing Binary?

1987 Epsilon Aurigae “model” from web site -->

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Page 19: Introduction to Binary Stars Steve B. Howell NOAO

The Oddest Eclipsing Binary Life??The Oddest Eclipsing Binary Life??

Elemarkhorsaurus from the Epsilon Aurigae Binary Star System

Caption: Ashraf, do you want to meet my new pet? Look, he is behind you and friendly. He loves the climate and his new home in the Eps Aur binary system. (From flickr)

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