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Results 81-90 of 465 (Search time: 0.012 seconds).
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Issue DateTitleAuthor(s)Citation
20-Aug-2001Very large array observations of the H92α line from NGC 5253 and Henize 2-10: Ionized gas around super star clustersMohan, Niruj R.; Anantharamaiah, K.R.; Goss, W.M.Astrophysical Journal, 2001, Vol.557, p659-670
20-Mar-2001Vacuum gaps in pulsars and PSR J2144-3933Gil, Janusz; Mitra, D.Astrophysical Journal, 2001, Vol.550, p383-391
20-Oct-2000On cooling flows and the Sunyaev-Zeldovich effectMajumdar, Subhabrata; Nath, Biman B.Astrophysical Journal, 2000, Vol.542, p597-607
10-Mar-2001The central velocity field in NGC 253: possible indication of a barDas, Mousumi; Anantharamaiah, K.R.; Yun, M.S.Astrophysical Journal, 2001, Vol.549, p896-905
1-Nov-2000Power spectrum of the density of cold atomic gas in the galaxy toward Cassiopeia A and Cygnus ADeshpande, A.A.; Dwarakanath, K.S.; Goss, W.M.Astrophysical Journal, 2000, Vol.543, p227-234
20-Jan-2001Upper limits on periodic, pulsed radio emission from the x-ray point source in Cassiopeia AMcLaughlin, M.A.; Cordes, J.M.; Deshpande, A.A.; Gaensler, B.M.; Hankins, T.H.; Kaspi, V.M.; Kern, J.S.Astrophysical Journal, 2001, Vol.547, pL41-44
1-Aug-2002Very large array detection of radio recombination lines from the radio nucleus of NGC 253: Ionization by a weak active galactic nucleus, an obscured super star cluster, or a compact supernova remnant?Mohan, Niruj R.; Anantharamaiah, K.R.; Goss, W.M.Astrophysical Journal, 2002, Vol.574, p701-708
1-Oct-2000Rapidly Rotating Strange Stars for a New Equation of State of Strange Quark MatterBombaci, Ignazio; Thampan, Arun V.; Datta, BhaskarThe Astrophysical Journal, 2000, Volume 541, Issue 2, pp. L71-L74
20-Feb-2000Conversion of neutron stars to strange stars as the central engine of gamma-ray burstsBombaci, Ignazio; Datta, BhaskarThe Astrophysical Journal, Volume 530, Issue 2, pp. L69-L72
Sep-2004Entropy of the intracluster medium at high redshiftNath, Biman B.Monthly Notices of the Royal Astronomical Society, 2004, Vol.353, Issue 3, p941-946.

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