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1.
Nature ; 551(7679): 210-213, 2017 11 08.
Article in English | MEDLINE | ID: mdl-29120417

ABSTRACT

Every supernova so far observed has been considered to be the terminal explosion of a star. Moreover, all supernovae with absorption lines in their spectra show those lines decreasing in velocity over time, as the ejecta expand and thin, revealing slower-moving material that was previously hidden. In addition, every supernova that exhibits the absorption lines of hydrogen has one main light-curve peak, or a plateau in luminosity, lasting approximately 100 days before declining. Here we report observations of iPTF14hls, an event that has spectra identical to a hydrogen-rich core-collapse supernova, but characteristics that differ extensively from those of known supernovae. The light curve has at least five peaks and remains bright for more than 600 days; the absorption lines show little to no decrease in velocity; and the radius of the line-forming region is more than an order of magnitude bigger than the radius of the photosphere derived from the continuum emission. These characteristics are consistent with a shell of several tens of solar masses ejected by the progenitor star at supernova-level energies a few hundred days before a terminal explosion. Another possible eruption was recorded at the same position in 1954. Multiple energetic pre-supernova eruptions are expected to occur in stars of 95 to 130 solar masses, which experience the pulsational pair instability. That model, however, does not account for the continued presence of hydrogen, or the energetics observed here. Another mechanism for the violent ejection of mass in massive stars may be required.

2.
Biochim Biophys Acta ; 1623(1): 21-8, 2003 Sep 08.
Article in English | MEDLINE | ID: mdl-12957713

ABSTRACT

Previous studies have described the isolation of a new metalloprotease with a strict specificity for the amide bonds of peptide substrates having a threonine residue at the P1' position [Biochem. Biophys. Res. Commun. 256 (1999) 307]. The present work reports the physico-chemical properties of the enzyme which enable the optimal conditions for the digestion of proteins by the protease to be determined. At pH 8.2 and up to 37 degrees C, the enzyme possesses a good proteolytic activity and is stable for at least 12 h. The protease is sensitive to detergents and dithiol-reducing agents so that these chemicals must be eliminated after treatment of the protein substrate when this needs to be denatured and reduced before its hydrolysis by the enzyme. An increase in the enzymatic activity is observed in the presence of urea up to a 2.0 M concentration, beyond which the activity decreases. The enzyme can also be used in the presence of organic solvents such as acetonitrile, isopropanol or dioxane (10%, v/v) without loss of activity. Studies performed with antibodies raised against the purified endoprotease Thr-N indicated the absence of cross-immunoinactivation and cross-immunoprecipitation with all tested proteases. Also, no homology of sequence was found with the proteases indexed in the databases. Thus, our results show that endoprotease Thr-N not only represents an original protease by its unique specificity but also by its immunological and molecular properties.


Subject(s)
Endopeptidases/chemistry , Endopeptidases/immunology , Metalloproteases/chemistry , Metalloproteases/immunology , Amino Acid Sequence , Animals , Endopeptidases/genetics , Endopeptidases/isolation & purification , Enzyme Activation , Enzyme Stability , Hydrogen-Ion Concentration , Metalloproteases/genetics , Metalloproteases/isolation & purification , Molecular Sequence Data , Molecular Weight , Rabbits , Sequence Analysis, Protein , Snails/chemistry , Snails/enzymology , Temperature
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