With the FUSE(Formal User interface Speciication Environment){System we present a methodology and a set of integrated tools for the automatic generation of graphical user interfaces. FUSE provides tool{based support for all phases (task{, user{, problem domain analysis, design of the logical user interface, design of user interface in a particular layout style) of the user interface development...

The c-myc regulatory region includes binding sites for a large set of transcription factors. The present studies demonstrate that in the absence of FBP [far upstream element (FUSE)-binding protein], which binds to the single-stranded FUSE, the remainder of the set fails to sustain endogenous c-myc expression. A dominant-negative FBP DNA-binding domain lacking effector activity or an antisense F...

A significant fraction of baryons in galaxies are the form diffuse gas circumgalactic medium (CGM). One critical component multi-phases CGM, so-called "coronal" warm-hot phase ($\rm 10^{5}-10^{6}$ K) traced by O VI 1031.93, 1037.62 \r{A} resonance lines, has rarely been detected emission from galaxy halos other than Milky Way. Here we report four additional detections nearby edge-on galaxies, N...

The far upstream element (FUSE) of the human c-myc proto-oncogene stimulates expression in undifferentiated cells. A FUSE-binding protein (FBP) is present in undifferentiated but not differentiated cells. Peptide sequences from the purified protein allowed cloning of cDNAs encoding FBP. Expression of FBP mRNA declined upon differentiation, suggesting transcriptional regulation of FBP. Features ...

The Far Ultraviolet Spectroscopic Explorer (FUSE) is a NASA astronomy mission that will explore the 905–1187Å wavelength region at high spectral resolution. Funded by NASA’s Explorer Program, this Origins mission is scheduled for a 1999 launch and at least three years of operations. The development of FUSE is being led by the Johns Hopkins University, with major contributions to the program fro...

We present new Far Ultraviolet Spectroscopic Explorer (FUSE) observations of Mira A’s wind-accreting companion star, Mira B. We find that the strongest lines in the FUSE spectrum are H2 lines fluoresced by H I Lyα. A previously analyzed Hubble Space Telescope (HST) spectrum also shows numerous Lyα-fluoresced H2 lines. The HST lines are all Lyman band lines, while the FUSE H2 lines are mostly We...