[astro-ph.EP] We present a radial velocity analysis of three bright, low-activity stars identified by the Dispersed Matter Planet Project (DMPP).
![Monte Carlo period simulations for each target. The v sin i values derived from species are used for randomly oriented (sinusoidally distributed) axial inclinations (green) and for a fixed i = 90o (light grey). The respective curves using the M16 v sin i estimates are also shown (orange and dark grey). The modal periods, Pˆ, are shown for each distribution. -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Three-new.png?resize=1200%2C622&ssl=1)
[astro-ph.EP] We present a radial velocity analysis of three bright, low-activity stars identified by the Dispersed Matter Planet Project (DMPP).