2010MNRAS.402L..21C


Query : 2010MNRAS.402L..21C

2010MNRAS.402L..21C - Mon. Not. R. Astron. Soc., 402, L21-L24 (2010/February-2)

Weak microlensing.

COLES J., SAHA P. and SCHMID H.M.

Abstract (from CDS):

A nearby star having a near-transit of a galaxy will cause a time-dependent weak lensing of the galaxy. Because the effect is small, we refer to this as weak microlensing. This could provide a useful method to weigh low-mass stars and brown dwarfs. We examine the feasibility of measuring masses in this way and find that a star causes measurable weak microlensing in a galaxy even at 10 Einstein radii away. Of the order of 1 mag I ≤ 25 galaxy comes close enough to one or the other of the ∼100 nearest stars per year.

Abstract Copyright: © 2009 The Authors. Journal compilation © 2009 RAS

Journal keyword(s): gravitational lensing - methods: statistical - stars: low-mass, brown dwarfs

CDS comments: 2MASS J0415+0935 is a misprint for 2MASS J0415-0935, DENIS 0255+4700 is a misprint for DENIS 0255-4700

Simbad objects: 9

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Number of rows : 9
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 DENIS J025503.3-470049 BD* 02 55 03.6927058871 -47 00 51.356903955     22.921 19.906 17.454 L9 170 0
2 2MASSI J0415195-093506 BD* 04 15 19.54368 -09 35 06.6732           T8.0 182 0
3 * alf CMa SB* 06 45 08.91728 -16 42 58.0171 -1.51 -1.46 -1.46 -1.46 -1.43 A0mA1Va 1610 0
4 * alf CMi SB* 07 39 18.11950 +05 13 29.9552 0.82 0.79 0.37 -0.05 -0.28 F5IV-V+DQZ 1925 0
5 * alf Cen B PM* 14 39 35.06311 -60 50 15.0992 2.89 2.21 1.33     K1V 1092 2
6 * alf Cen A SB* 14 39 36.49400 -60 50 02.3737 0.96 0.72 0.01     G2V 1352 1
7 GJ 570 D BD* 14 57 14.96256 -21 21 47.7504           T8 242 1
8 SCR J1845-6357B BD* 18 45 05.2560 -63 57 47.808           T6 35 0
9 * alf Aql dS* 19 50 46.99855 +08 52 05.9563 1.07 0.98 0.76 0.62 0.49 A7Vn 919 1

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