Abstract
A detailed discussion is given of the possibility of determining peculiar velocities of clusters of galaxies by measuring the kinematic Sunyaev-Zeldovich effect. From available optical and X-ray data we select a sample of clusters for which the effect might be measurable at the optimal frequency where the thermal Sunyaev-Zeldovich effect vanishes.
| Original language | English |
|---|---|
| Pages (from-to) | 21-24 |
| Number of pages | 4 |
| Journal | Astrophysical Journal |
| Volume | 372 |
| Issue number | 1 |
| DOIs | |
| State | Published - 1 May 1991 |
Keywords
- Cosmic background radiation
- Galaxies: clustering
- Galaxies: redshifts