We have used 3D-HST spectra to measure redshifts and Hα equivalent widths (EWHα) for a complete, stellar mass-limited sample of 34 galaxies at 1 < z < 1.5 with M star > 1011?M ☉ in the COSMOS, GOODS, and AEGIS fields. We find that a substantial fraction of massive galaxies ...
Absence of a Spin Gap in the materials. Superconducting Ladder Compound Sr2Cal 2 C ~ 2 4 0 4 , suhst~tation.The structure of Sr,,Cu,,OIIK. pa'sibl~ ascribcJ t,> the P clcrcnLience t c r ~ o~t~a scorrclatccl T L > I I I ~ > I I ~ ~ ...
We discuss its structure, in latitude and longitude, and show that it is consistent with precipitation by pitch angle scattering. Fainter concentric narrow ovals are also present on the north polar cap, presumably at the footprint of open field lines. Both polar caps are partly covered by a ...
The input energy flux in this spots is huge and variable (0.8–5 × 1011W).WileyJOURNAL OF GEOPHYSICAL RESEARCHPrangé, R., D. Rego, L. Pallier, J. Connerney, and P. Zarka: 1998, ‘Detailed study of FUV Jovian auroral Features with the post-COSTAR HST faint object camera’. J. ...
Atmospheres, StructureThe nature and mechanisms producing the chromophore agents that provide color to the upper clouds and hazes of the atmospheres of the giant planets are largely unknown. In recent times, the changes in red coloration that have occurred in large- and medium-scale Jovian ...