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Browsing by Author "Robin, A. C."

Browsing by Author "Robin, A. C."

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  • Creze, M.; Mohan, V.; Robin, A. C.; Reyle, C.; Mc Cracken, H. J.; Cuillandre, J. C.; Le Fevre, O.; Mellier, Y. (2004)
    Having ruled out the possibility that stellar objects are the main contributor of the dark matter embedding galaxies, microlensing experiments cannot exclude the hypothesis that a significant fraction of the MilkyWay dark ...
  • Robin, A. C.; Creze, M.; Mohan, V. (1992)
    As part of a stellar population sampling program, a series of photometric probes at various field sizes and depths have been obtained in a low-extinction window in the Galactic anticenter direction. Such data set strong ...
  • Bienayme, O.; Mohan, V.; Creze, M.; Considere, S.; Robin, A. C. (1992)
    A sample survey is being conducted in UBV photometry and proper motions as part of an investigation of galactic structure and evolution. In the present paper we discuss the observational results in a restricted field (1.78 ...
  • Ojha, D. K.; Bienayme, O.; Mohan, V.; Robin, A. C. (1999)
    A photometric and proper motion survey has been obtained in 2 directions at intermediate latitude: (l = 167.5° , b = 47.4° ; α₂ₒₒₒ= 9ʰ 41ᵐ 26ᶳ ,δ₂ₒₒₒ = +49° 53' 27” ) and (l = 278° , b = 47° ; α₂ₒₒₒ = 11ʰ 42ᵐ 56ᶳ , δ₂ₒₒₒ ...
  • Robin, A. C.; Creze, M.; Mohan, V. (1992)
    Three colour photometry on CCD frames in the Special Ares SpA23 provides a deep probe of the galactic disc in a low absorption window towards the anticenter. Magnitudes to better than 10% at V = 25 and B – V colour down ...
  • Mohan, V.; Sanwal, B. B.; Paliwal, D. C.; Pandey, A. K.; Bhatt, B. C.; Robin, A. C. (1996)
    Using CCD observations, photometric magnitudes have been obtained in two galactic directions at intermediate latitude. A total of 7 sub-fields in one direction (l = 3°, b = 47°) have been observed leading to photometric ...
  • Mohan, V.; Ojha, D. K.; Bienayme, O.; Paliwal, D. C.; Pandey, A. K.; Robin, A. C.; Chareton, M.; Bhatt, B. C.; Sanwal, B. B.; Oblak, E.; Haywood, M.; Creze, M. (1994)
    Using CCD observations photometric magnitudes have been obtained in 18 sub-fields in a direction at intermediate galactic latitude (l = 170°, b = 45°) in a 14 deg² area. B and V magnitudes have been obtained for a total ...

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