Gravitational microlensing by the dark halo of M31
| dc.creator | Jetzer, Philippe | |
| dc.date | 1993-11-18 | |
| dc.date | 1993-11-19 | |
| dc.date.accessioned | 2026-07-07T08:58:12Z | |
| dc.date.available | 2026-07-07T08:58:12Z | |
| dc.description | It has been shown by Paczyński that gravitational microlensing is potentially a useful method for detecting the dark constituents of the halo of our galaxy, if their mass lies in the approximate domain $10^{-6}<M/M_\odot<10^{-1}$. Microlensing observations now im progress monitor several millions of stars in the Large Magellanic Cloud and in the Galactic Bulge. Here I discuss the main features of the microlensing events: in particular their rates and probability. | |
| dc.description | 4, latex, ZU-TH 27/93 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9311045 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9311045 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/147232 | |
| dc.subject | Astrophysics | |
| dc.title | Gravitational microlensing by the dark halo of M31 | |
| dc.type | text |