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Search for Microlensing Events Towards M31 Galaxy

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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 2008-05-17T10:12:23Z
dc.date.available 2008-05-17T10:12:23Z
dc.date.issued 2001
dc.identifier.citation BASI, Vol. 29, No. 4, pp. 531 - 544 en
dc.identifier.uri http://hdl.handle.net/2248/2324
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, Nainital, India. The observations have been accumulated for about hundred 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
dc.format.extent 1169194 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Astronomical Society of India en
dc.relation.uri http://adsabs.harvard.edu/abs/2001BASI...29..531J en
dc.subject Galaxy:halo en
dc.subject Cosmology:gravitational microlensing en
dc.subject Galaxies:M31 en
dc.subject Pixel technique:variable star en
dc.title Search for Microlensing Events Towards M31 Galaxy en
dc.type Article en


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