1999ApJ...525..734G


Query : 1999ApJ...525..734G

1999ApJ...525..734G - Astrophys. J., 525, 734-736 (1999/November-2)

A new argument against an intervening stellar population toward the Large Magellanic Cloud.

GOULD A.

Abstract (from CDS):

Zaritsky & Lin have claimed detection of an intervening population of stars toward the Large Magellanic Cloud (LMC), which, they believe, could account for a substantial fraction of the observed microlensing events. I show that the observed timescales of these events imply that if such an intervening population were composed of ordinary stars that gave rise to a significant fraction of the microlensing events, then the population could not be associated with the LMC. I present two independent statistical arguments which together essentially rule out such a chance alignment of unassociated structures. On the other hand, if the intervening structure is associated with the LMC, I show that of order half the mass in this structure is in substellar objects, which would make it unlike any known stellar population.

Abstract Copyright: ∼

Journal keyword(s): Cosmology: Dark Matter - Galaxy: Halo - Cosmology: Gravitational Lensing - Galaxies: Magellanic Clouds

Simbad objects: 15

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Number of rows : 15
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 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 12317 1
2 NAME Sculptor Dwarf Galaxy G 01 00 09.4 -33 42 32   9.79 8.6 8.81   ~ 1498 4
3 MCG-06-07-001 G 02 39 59.3 -34 26 57   9.02 7.4     ~ 1894 1
4 NAME E 1 GlC 03 55 02.5 -49 36 52           ~ 229 0
5 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 19090 0
6 ESO 206-20A G 06 41 36.7 -50 57 58   22.14 11.0 19.47   ~ 1190 0
7 NGC 2419 GlC 07 38 08.51 +38 52 54.9     10.05     ~ 998 0
8 NAME Sextans C GlC 10 05 30.96 +00 04 15.4   15.5 13.9     ~ 354 1
9 Z 64-73 G 10 08 28.12 +12 18 23.4   11.3 10.0     ~ 1284 1
10 MCG-01-26-030 H2G 10 11 00.5 -04 41 30 12.48 12.13 11.93 11.78   ~ 789 2
11 Z 126-111 G 11 13 28.13 +22 09 10.1   12.9 12.0     ~ 899 0
12 GCl 17 GlC 11 29 16.80 +28 58 25.0   14.4       ~ 379 1
13 Z 318-18 G 15 09 08.0 +67 13 21   13.60 10.6     ~ 1459 0
14 GCl 38 GlC 16 10 59.00 +14 57 42.0           ~ 399 0
15 Z 300-12 G 17 20 14.335 +57 55 16.39   12.40 10.6     ~ 1428 1

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