LX Li,B Paczyński
LX Li
The highest efficiency of converting rest mass into energy by accreting matter into a Kerr black hole is approximately 31% (Thorne 1974). We propose a new process in which periods of accretion from a thin disk, and the associated spin-up of...
H Umeda,K Nomoto,S Tsuruta et al.
H Umeda et al.
Very recently the Chandra first light observation discovered a point-like source in the Cassiopeia A supernova remnant. This detection was subsequently confirmed by the analyses of the archival data from both ROSAT and Einstein observations...
A Model for the Quiescent Phase of the Recurrent Nova U Scorpii [0.03%]
UC sco的名字为UScorpii，简称U_Sco。淬灭期指的是复发新星经历大爆发之后的宁静期。题目可以翻译为“大爆发型复发新星USco的淬灭期模型”。此题目的翻译建议为：“复发新星UC Sco的静默期模型”
I Hachisu I,M Kato,T Kato et al.
I Hachisu I et al.
A theoretical light curve is constructed for the quiescent phase of the recurrent nova U Scorpii in order to resolve the existing distance discrepancy between the outbursts (d approximately 6 kpc) and the quiescences (d approximately 14 kpc...
Evolutionary Timescale of the Pulsating White Dwarf G117-B15A: The Most Stable Optical Clock Known [0.03%]
脉动白矮星G117-B15A的演化时间标尺：已知最稳定的光学时钟
SO Kepler,A Mukadam,DE Winget et al.
SO Kepler et al.
We observe G117-B15A, the most precise optical clock known, to measure the rate of change of the main pulsation period of this blue-edge DAV white dwarf. Even though the obtained value is only within 1 sigma, P&d2;=&parl0;2.3+/-1.4&parr0;x1...
Discovery of a New Pulsating X-Ray Source with a 1549.1 Second Period, AX J183220-0840 [0.03%]
1549.1秒新周期变源AX J183220-0840的发现
M Sugizaki,K Kinugasa,K Matsuzaki et al.
M Sugizaki et al.
A new pulsating X-ray source, AX J183220-0840, with a 1549.1 s period was discovered at R.A.=18h32m20s and decl.=-8&j0;40'30" (J2000, with an uncertainty of 0&farcm;6) during an ASCA observation on the Galactic plane. The source was observe...
First Mass-resolved Measurement of High-Energy Cosmic-Ray Antiprotons [0.03%]
首次太空中高能宇宙射线反质子质量分辨谱的测量
D Bergström,M Boezio,P Carlson et al.
D Bergström et al.
We report new results for the cosmic-ray antiproton-to-proton ratio from 3 to 50 GeV at the top of the atmosphere. These results represent the first measurements, on an event-by-event basis, of mass-resolved antiprotons above 18 GeV. The re...
Detection of Polarized Millimeter and Submillimeter Emission from Sagittarius A* [0.03%]
半人马座A*毫秒和亚毫米级辐射偏振探测
DK Aitken,J Greaves,A Chrysostomou et al.
DK Aitken et al.
We report the detection of linear polarization from Sgr A* at 750, 850, 1350, and 2000 µm which confirms the contribution of synchrotron radiation. From the lack of polarization at longer wavelengths, it appears to arise in the millimeter/...
Large Magellanic Cloud Planetary Nebula Morphology: Probing Stellar Populations and Evolution [0.03%]
大麦哲伦云行星状星云的形态：探究恒星种群与演化
L Stanghellini,RA Shaw,B Balick et al.
L Stanghellini et al.
Planetary nebulae (PNe) in the Large Magellanic Cloud (LMC) offer the unique opportunity to study both the population and evolution of low- and intermediate-mass stars, by means of the morphological type of the nebula. Using observations fr...
J Granot,T Piran,R Sari
J Granot
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 de...
Multiple Sub-Jet Model of Gamma-Ray Bursts and Possible Origin of X-Ray Precursors and Postcursors [0.03%]
伽玛射线暴的多重子喷流模型及其X射线前驱和后随辐射的可能起源
T Nakamura
T Nakamura
We assume that internal shocks of gamma-ray bursts (GRBs) consist of multiple sub-jets with a collimation half-angle of about several times gamma-1i, where gammai is the Lorentz factor of each sub-jet. If by chance a sub-jet is first emitte...