The N-terminal 209-aa domain of high molecular- weight 4.1R isoforms abrogates 4.1R targeting to the nucleus

An extensive repertoire of protein 4.1R isoforms is predominantly generated by alternative pre-mRNA splicing and differential usage of two translation initiation sites. The usage of the most upstream ATG (ATG-1) generates isoforms containing N-terminal extensions of up to 209 aa compared with those translated from the downstream ATG (ATG-2). To characterize nonerythroid 4.1R proteins translated from ATG-1 and analyze their intracellular localization, we cloned 4.1R cDNAs containing this translation initiation site. Six different clones were isolated from the nucleated human MOLT-4 T-cell line by reverse transcriptase–PCR techniques. Transient expression of the six ATG-1-translated 4.1R isoforms tagged with a c-Myc epitope revealed that all of them predominantly distributed to the plasma membrane and the endoplasmic reticulum. Staining of MOLT-4 cell plasma membranes but not nuclei was also observed by immunofluorescence microscopy by using an antibody specific to the N-terminal extension. Consistent with this, the antibody reacted with a major endogenous protein of ≈145 kDa present in nonnuclear but absent from nuclear fractions prepared from MOLT-4 cells. Because these data suggested that ATG-1-translated 4.1R isoforms were predominantly excluded from the nucleus, we fused the 209-aa domain to nuclear 4.1R isoforms encoded from ATG-2 and observed that this domain inhibited their nuclear targeting. All these results indicate that the N-terminal domain of ATG-1-translated 4.1R isoforms plays a pivotal role in differential targeting of proteins 4.1R.

Structure and evolution of the compact radio source in NGC 1275.

Investigations of the fine-scale structure in the compact nucleus of the radio source 3C 84 in NGC 1275 (New General Catalogue number) are reported. Structural monitoring observations beginning as early as 1976, and continuing to the present, revealed subluminal motions in a jet-like relatively diffuse region extending away from a flat-spectrum core. A counterjet feature was discovered in 1993, and very recent nearly simultaneous studies have detected the same feature at five frequencies ranging from 5 to 43 GHz. The counterjet exhibits a strong low-frequency cutoff, giving this region of the source an inverted spectrum. The observations are consistent with a physical model in which the cutoff arises from free-free absorption in a volume that surrounds the core but obscures only the counterjet feature. If such a model is confirmed, very-long-baseline radio interferometry observations can then be used to probe the accretion region, outside the radio jet, on parsec scales.