A new gamma-ray burst classification scheme from GRB 060614

Gamma-ray bursts (GRBs) are known to come in two duration classes, separated at approximately 2 s. Long-duration bursts originate from star-forming regions in galaxies, have accompanying supernovae when these are near enough to observe and are probably caused by massive-star collapsars. Recent observations show that short-duration bursts originate in regions within their host galaxies that have lower star-formation rates, consistent with binary neutron star or neutron star-black hole mergers. Moreover, although their hosts are predominantly nearby galaxies, no supernovae have been so far associated with short-duration GRBs. Here we report that the bright, nearby GRB 060614 does not fit into either class. Its approximately 102-s duration groups it with long-duration GRBs, while its temporal lag and peak luminosity fall entirely within the short-duration GRB subclass. Moreover, very deep optical observations exclude an accompanying supernova, similar to short-duration GRBs. This combination of a long-duration event without an accompanying supernova poses a challenge to both the collapsar and the merging-neutron-star interpretations and opens the door to a new GRB classification scheme that straddles both long- and short-duration bursts.

An expanding radio nebula produced by a giant flare from the magnetar SGR 1806–20

Soft gamma-ray repeaters (SGRs) are 'magnetars', a small class of slowly spinning neutron stars with extreme surface magnetic fields, B approximately 10(15) gauss (refs 1 , 2 -3). On 27 December 2004, a giant flare was detected from the magnetar SGR 1806-20 (ref. 2), only the third such event recorded. This burst of energy was detected by a variety of instruments and even caused an ionospheric disturbance in the Earth's upper atmosphere that was recorded around the globe. Here we report the detection of a fading radio afterglow produced by this outburst, with a luminosity 500 times larger than the only other detection of a similar source. From day 6 to day 19 after the flare from SGR 1806-20, a resolved, linearly polarized, radio nebula was seen, expanding at approximately a quarter of the speed of light. To create this nebula, at least 4 x 10(43) ergs of energy must have been emitted by the giant flare in the form of magnetic fields and relativistic particles.

A giant γ-ray flare from the magnetar SGR 1806–20

Two classes of rotating neutron stars-soft gamma-ray repeaters (SGRs) and anomalous X-ray pulsars-are magnetars, whose X-ray emission is powered by a very strong magnetic field (B approximately 10(15) G). SGRs occasionally become 'active', producing many short X-ray bursts. Extremely rarely, an SGR emits a giant flare with a total energy about a thousand times higher than in a typical burst. Here we report that SGR 1806-20 emitted a giant flare on 27 December 2004. The total (isotropic) flare energy is 2 x 10(46) erg, which is about a hundred times higher than the other two previously observed giant flares. The energy release probably occurred during a catastrophic reconfiguration of the neutron star's magnetic field. If the event had occurred at a larger distance, but within 40 megaparsecs, it would have resembled a short, hard gamma-ray burst, suggesting that flares from extragalactic SGRs may form a subclass of such bursts.

The Synchrotron Spectrum of Fast Cooling Electrons Revisited

We discuss the spectrum arising from synchrotron emission by fast cooling (FC) electrons, when fresh electrons are continually accelerated by a strong blast wave, into a power-law distribution of energies. The FC spectrum has so far been described by four power-law segments divided by three break frequencies nusa<nuc<num. This is valid for a homogeneous electron distribution. However, hot electrons are located right after the shock, while most electrons are farther downstream and have cooled. This spatial distribution changes the optically thick part of the spectrum, introducing a new break frequency, nuac<nusa, and a new spectral slope, Fnu~nu11&solm0;8 for nuac<nu<nusa. The familiar Fnu~nu2 holds only for nu<nuac. This ordering of the break frequencies is relevant for typical gamma-ray burst (GRB) afterglows in an interstellar medium environment. Other possibilities arise for internal shocks or afterglows in dense circumstellar winds. We discuss the possible implications of this spectrum for GRBs and their afterglows in the context of the internal-external shock model. Observations of Fnu~nu11&solm0;8 would enable us to probe scales much smaller than the typical size of the system and to constrain the amount of turbulent mixing behind the shock.

Sodium imaging of human body organs and extremities in vivo

In vivo sodium magnetic resonance (MR) images of various structures--such as the heart, chest wall, kidneys, spine, liver, gallbladder, breasts, knees, hands, and feet--were obtained at 1.9 T. Improved sensitivity relative to standard spin-echo imaging was achieved with use of a modified three-dimensional acquisition sequence with short repetition and gradient-echo times (45 and 6.4 msec, respectively) and with use of special cylindrical and planar radio-frequency coils. Imaging times of 2-30 minutes were sufficient to render good-quality images with high contrast sensitivity. Relatively strong sodium signals were found to emanate from such sources as cerebrospinal fluid, blood serum, interstitial fluid, joint fluid, and cartilage. It is concluded that sodium imaging of body organs and extremities is feasible and is potentially of clinical diagnostic value, as is the more extensively studied sodium imaging of the head.

1H NMR relaxation studies of the hydrogen-bonded imino protons of poly(dA-dT)

Measurements on the thymine imino proton relaxation rates have been used to study various structural and dynamic properties of 53 +/- 15 base pair long poly(dA-dT). Below 10 degrees C, the relaxation is dominated by dipolar magnetic interactions. At 1 degrees C the relaxation of the transverse magnetization is exponential (R2 = 124 s-1), but the relaxation of longitudinal magnetization is highly nonexponential due to spin-diffusion effects (initial decay rate constant of 28 s-1 and a slower rate of approximately 2.5 s-1 after equilibration of spin polarization). Neither a rigid-rod model nor simple wormlike motions can account for the observed low-temperature relaxation behavior. However, when localized internal motions of the base pairs (three-state jump model) are allowed for, a good fit of the experimental data is obtained by using a correlation time for internal motion of 7 X 10(-10) s and an angular displacement of the bases of +/- 32 degrees relative to the helix axis. The observed R2/R1 ratio for the thymine imino proton yields a value of 1.14 +/- 0.08 A for the imino proton nitrogen distance. Nuclear Overhauser effect (NOE) measurements establish that the base pairing in poly(dA-dT) is Watson-Crick in solution and not Hoogsteen. Exchange of the T-imino protons with H2O dominates the longitudinal relaxation above 28 degrees C (activation energy of 17 +/- 2 kcal and an exchange rate of 5 +/- 2 s-1 at 300 K). Similar values have been reported for the A X T base pairs in DNA restriction fragments and for A X U base pairs in poly(A) X poly(U). These observations can be explained by a model in which exchange of T-imino protons occurs as a result of a single base pair opening, with a rate that is approximately independent of nearest-neighbor sequences and DNA length. Our observations appear to be inconsistent with a soliton model of proton exchange.

Magnetic resonance measurements of intersubstrate distances at the active site of protein kinase using substitution-inert cobalt(III) and chromium(III) complexes of adenosine 5'-(beta, gamma-methylenetriphosphate)

Co3+ and Cr3+ complexes of beta, gamma-methylene-ATP (AMPPCP), which are substitution-inert substrate analogues inactive in phosphoryl transfer reactions, have been used in binding and structural studies of cAMP-dependent protein kinase. Dissociation constants of enzyme complexes with Co(NH3)4AMPPCP and CrAMPPCP and with Mn2+, which binds at an inhibitory site, were determined by electron paramagnetic resonance and by proton relaxation rate enhancement techniques. Nuclear relaxation rate measurements at 100 and 360 MHz were used to determine the distance between Mn2+ and the beta, gamma-methylene protons of Co-(NH3)4AMPPCP, yielding 7.4 +/- 0.6 A in the absence of enzyme and 5.0 +/- 0.9 A when both Mn2+ and Co-(NH3)4AMPPCP were bound to the enzyme. The effect of the paramagnetic CrAMPPCP on the electron spin relaxation time of the enzyme-bound Mn2+ was used used to calculate the distance between the two metal ions of 4.8 +/- 0.4 A. This distance and the Mn2+-methylene distance are consistent with the previous finding that the inhibitory metal bridges the enzyme to the triphosphate chain of the enzyme-bound nucleotide [Granot, J., Kondo, H., Armstrong, R. M., Mildvan, A. S., & Kaiser, E. T. (1979) Biochemistry 18, 2339]. From the paramagnetic effects on the relaxation rates of the protons of the peptide substrate Leu-Arg-Arg-Ala-Ser-Leu-Gly, distances from Mn2+ and Cr3+ to the serine methylene protons of 9.1 +/- 0.9 and 8.1 +/- 0.8 A, respectively, were calculated. These and previous measurements were used to estimate a distance of 5.3 +/- 0.7 A along the reaction coordinate between the gamma-phosphorus of ATP and the serine hydroxyl oxygen. This distance is 2 A greater than that required for molecular contact. The mechanistic implications of these findings are discussed.

Structural and exchange properties of "Co(III)-phenanthroline-ATP": a labeling reagent for the active site of ATPases

This paper reports on 1H and 31P NMR as well as EPR measurements of the labeling reagent of ATPase sites, "Co(III)-(phen)-ATP." This complex is found to be paramagnetic, as deduced both from its EPR spectrum and from the significant broadening, though almost unshifted, proton and phosphorus resonances. This paramagnetism is a result of the incorporation of the superoxide free-radical anion in the coordination sphere of the trivalent cobalt ion. Evidence for the presence of superoxide in the complex is based on competition experiments with cyanide, which is able to displace the superoxide anion. The latter was identified by its inducing effect on the photoreactivity of luminol. The displacement of superoxide by cyanide was accompanied by the abolition of the paramagnetism of the complex. The relative distances between the protons and phosphorus atoms of ATP and the superoxide anion in the complex were calculated using the NMR line-broadening data. Structural models compatible with the experimental results are proposed. Under conditions of excess of adenine nucleotides or phenanthroline, the coordinated ATP molecule becomes exchangeable. This phenomenon is attributed to the labilization of the cobaltic ion ligands induced by the superoxide anion.

Nuclear magnetic resonance studies of 6-hydroxydopamine and its interactions with SH-containing model compounds. Evaluation of possible mechanism for neurocytotoxicity

6-Hydroxydopamine (I) is a well-known neurocytotoxic agent which has become an important tool in many neurochemical studies in recent years. Biochemical investigations of the mechanism of action of 6-hydroxydopamine indicated that this amine binds covalently and irreversibly to proteins. In the present work, molecular properties of 6-hydroxydopamine in aqueous solution such as self-association, ionization, intramolecular conformations, and possible cyclization were investigated using 1H nuclear magnetic resonance spectroscopy. A model study for the interaction of 6-hydroxydopamine with proteins was undertaken by using SH-containing molecules: cysteine, glutathione, and bovine serum albumin. The binding of these compounds to 6-hydroxydopamine was found to cause labilization of the hydrogen attached to C2 of the amine aromatic ring. This effect was interpreted in terms of nucleophilic attack of RS- on C1 of 6-hydroxydopamine. A proposed model for neurocytotoxicity is discussed.