The microlensing events in Q2237+0305A: No case against small masses/large sources
| dc.creator | Haugan, S. V. H. | |
| dc.date | 1995-08-23 | |
| dc.date.accessioned | 2026-07-07T02:20:01Z | |
| dc.date.available | 2026-07-07T02:20:01Z | |
| dc.description | It is demonstrated that the 1988-90 microlensing events in image A of Q2237+0305 reported by Racine (1992) do not exclude microlensing models with very low average mass, making the source radius larger than the projected Einstein radius $η_0$ (Refsdal and Stabell 1991, 1993). This is contrary to what has been claimed by Witt and Mao (1994). Since these events are the best resolved microlensing events recorded in Q2237+0305, further work should not exclude the possibility of a large source when interpreting lightcurve data. | |
| dc.description | 2 pages, 1 figure. Uses crckapb.sty. To appear in the Proceedings of the IAU Symposium 173: ``Astrophysical Applications of Gravitational Lensing'', Kluwer Academic Publishers, Eds.: C. S. Kochanek and J. N. Hewitt. Also available through http://www.uio.no/~steinhh/index.html | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9508103 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9508103 | |
| dc.identifier | IAU Symp. 173 (1996) 255 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/10093 | |
| dc.subject | Astrophysics | |
| dc.title | The microlensing events in Q2237+0305A: No case against small masses/large sources | |
| dc.type | text |