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Results 41-50 of 98 (Search time: 0.01 seconds).
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Issue DateTitleAuthor(s)Citation
Feb-1991Radio pulsars and the scale height of ionized hydrogenBhattacharya, D.; Verbunt, F.Astronomy and Astrophysics, 1991, Vol.242, p128-132
Dec-2000On the origin of the difference between the runaway velocities of the OB-supergiant X-ray binaries and the Be/X-ray binariesvan den Heuvel, E.P.J.; Portegies Zwart, S.F.; Bhattacharya, D.; Kaper, L.Astronomy and Astrophysics, 2000, Vol.364, p563-572
Apr-2004Early optical and millimeter observations of GRB 030226 afterglowPandey, S.B.; Sagar, R.; Anupama, G.C.; Bhattacharya, D.; Sahu, D.K.; Castro-Tirado, A.J.; Bremer, M.Astronomy and Astrophysics, 2004, Vol.417, p919-924
Sep-2003The optical afterglow of the not so dark GRB 021211Pandey, S.B.; Anupama, G.C.; Sagar, R.; Bhattacharya, D.; Castro-Tirado, A.J.; Sahu, D.K.; Parihar, Padmakar; Prabhu, T.P.Astronomy and Astrophysics, 2003, Vol.408, pL21-L24
1-Apr-1999The effect of magnetic fields on bold gamma-ray bursts inferred from multi-wavelength observations of the burst of 23 January 1999Galama, T.J.; Briggs, M.S.; Wijers, R.A.M.J.; Bhattacharya, D.; et al.Nature, 1999, Vol.398, p394-399
13-Feb-1992Genesis of a pulsar's planetsWijers, R.A.M.J.; van den Heuvel, E.P.J.; van Kerkwijk, M.H.; Bhattacharya, D.Nature, 1992, Vol.355, p593
1996The case for no field decay from improved pulsar population studiesHartman, J.W.; Verbunt, F.; Bhattacharya, D.; Wijers, H.IAU Colloquium, 1996, Vol.160, p47
1996The origin of millisecond pulsarsBhattacharya, D.IAU Colloquium, 1996, Vol.160, p547
1994Models for the formation of binary and millisecond pulsarsBhattacharya, D.IAU Symposium, 1996, Vol.165, p243
1999Applications of radio pulsar population synthesisVerbunt, F.; Hartman, J.W.; Bhattacharya, D.; Wijers, R.A.M.J.; Nelemans, G.Proceedings of the Netherlands Academy Colloquim, 1999, p215

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