ARIES-Institutional Digital Repository

Search for microlensing events towards M31 galaxy

Show simple item record

dc.contributor.author Joshi, Y. C.
dc.contributor.author Pandey, A. K.
dc.contributor.author Narasimha, D.
dc.contributor.author Sagar, R.
dc.date.accessioned 2009-08-10T07:07:39Z
dc.date.available 2009-08-10T07:07:39Z
dc.date.issued 2001
dc.identifier.citation This article downloded from ADS Free Online Journal en_US
dc.identifier.uri http://hdl.handle.net/123456789/240
dc.description.abstract M31, the prominent galaxy of the Local Group, is located at a distance of about 700 kpc. Due to its convenient orientation, it is an alluring target for gravitational microlensing to search for massive astrophysical compact halo objects (MACHOs), in both the Galactic halo and its own halo. We have carried out the observations of the suburb of M31 galaxy using the 104-cm Sampurnanand Telescope of the State Observatory, Naini Tal, India. The observations have been accumulated for about hundered nights spanning over 800 days during 1998-2001. After the initial tests and preliminary analysis of the first two years data we have detected some possible M31 Cepheid variables of period between 10 to 85 days. Also using pixel method we have got an irregular variable and further analysis is in progress to detect the lensing events in the observed region. en_US
dc.language.iso en_US en_US
dc.relation.ispartofseries basi29-531
dc.subject Galaxy, Halo-cosmology, Gravitational microlensing-galaxies, M31-pixel technique, Variable stars en_US
dc.title Search for microlensing events towards M31 galaxy en_US
dc.type Article en_US


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search ARIES-IDR


Advanced Search

Browse

My Account

Context