Chapter 10 of 11 · 11 min read
Spectra and velocities
Doppler shifts, rotation curves and dynamical masses, binary orbits and the mass function, and expanding shells.
Doppler shifts
For ,
Positive means receding (redshift). For larger speeds, . Use the air wavelength when the data are in air (Hα at 6562.82 Å in air, 656.281 nm in the 2017 problem; follow the value the problem gives).
The 2017 galaxy spectra show shifts of only 0.1–0.2 nm on 656 nm, so keep all the decimals: a 0.001 nm reading error is 0.5 km/s.
Rotation curves and dark matter
For circular orbits in a spherical mass distribution,
Independent components add in quadrature: . A flat rotation curve ( constant) means , so at large radius. Visible matter alone would give (Keplerian) outside the light. The difference is the evidence for dark matter.
Binary stars and the mass function
For a star in a circular orbit with period and RV semi-amplitude :
The mass function is a lower limit on (it equals only if and ). To get you need and from elsewhere: and a radius give ; a rotation period and give if the rotation is synchronised.
If exceeds about 2.5 and the companion emits nothing, it is a black hole candidate (2018 D2).
Pulsars and accelerations
An orbiting pulsar's apparent spin period is Doppler shifted, , and the line-of-sight acceleration is measured from the drift of . For a circular orbit the pair traces an ellipse with semi-axes and , which is the basis of 2016 D1.
Expanding shells and P Cygni profiles
An expanding shell produces emission at the line's rest wavelength and blueshifted absorption from gas between us and the star: a P Cygni profile. The absorption minimum gives the expansion velocity. Integrating the velocity over time gives the shell's radius:
and with a distance, an angular size . The 2019 nova problem used this. A pulsating star works the same way, with (the projection factor ; the sign because a positive radial velocity means the surface is moving away from us, i.e. contracting).
Key formulas
- Doppler shift
- Enclosed mass
- Mass function
- Projected orbit
Common mistakes
- Forgetting to subtract the systemic velocity γ before integrating a velocity curve.
- Treating the mass function as the companion's mass.
- Mixing vacuum and air wavelengths.
- Adding velocity components linearly instead of in quadrature.
Practise this chapter
Past IOAA problems that use these skills.
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