1999A&A...344L..49A


Query : 1999A&A...344L..49A

1999A&A...344L..49A - Astronomy and Astrophysics, volume 344L49-52 (1999/4-2)

AgapeZ1: a large amplification microlensing event or an odd variable star towards the inner bulge of M31.

ANSARI R., AURIERE M., BAILLON P., BOUQUET A., COUPINOT G., COUTURES C., GHESQUIERE C., GIRAUD-HERAUD Y., GONDOLO P., HECQUET J., KAPLAN J., KIM A., LE DU Y., MELCHIOR A.L., MONIEZ M., PICAT J.P. and SOUCAIL G.

Abstract (from CDS):

AgapeZ1 is the brightest and the shortest duration microlensing candidate event found to date in the Agape experiment. It occurred only 42'' from the centre of M31 at RA=00:42:41.47 and Dec=+41°16'39.1" (J2000). Our photometry shows that the half intensity duration of the event is 5.3days and at maximum brightness its magnitude is R=17.9 (MR~-6) with B-R=0.80mag colour. A search on HST archives produced a single resolved star within the projected event position error box. Its magnitude is R=22, and its colour is compatible with that of the event at the 2 σ level. If this event is identified with the HST star, the implied amplification is about 4 magnitudes or 40 in brightness. This would lead to an Einstein crossing time radius of about 60 days. AgapeZ1 could be a bulge/bulge microlensing event involving a binary star. The photometric properties of the object are inconsistent with classical M31 variable stars such as Miras, classical novae, dwarf-novae, and bumpers. However, we cannot rule out the possibility that AgapeZ1 is in fact an odd variable star.

Abstract Copyright: ∼

Journal keyword(s): Galaxy: halo - cosmology: observations - cosmology: dark matter - cosmology: gravitational lensing

Nomenclature: AGAPE Z1 N=1.

Simbad objects: 2

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Number of rows : 2
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 AGAPE Z1 * 00 42 41.47 +41 16 39.1           ~ 2 1
2 M 31 AGN 00 42 44.330 +41 16 07.50 4.86 4.36 3.44     ~ 13622 1

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