Parallax of the IBEX Ribbon Indicates a Spatially-Retained Source [0.03%]
依巴克斯带状结构的视差表明其源自一处空间位置固定的源头
E J Zirnstein,P Swaczyna,D J McComas et al.
E J Zirnstein et al.
In 2009, the Interstellar Boundary Explorer (IBEX) discovered the existence of a narrow "ribbon" of intense energetic neutral atom (ENA) emission projecting approximately a circle in the sky. It is believed that the ribbon originates from o...
E J Zirnstein,P Swaczyna,D J McComas et al.
E J Zirnstein et al.
In 2009, the Interstellar Boundary Explorer (IBEX) discovered the existence of a narrow "ribbon" of intense energetic neutral atom (ENA) emission projecting approximately a circle in the sky. It is believed that the ribbon originates from o...
Strong Scattering of ~keV Pickup Ions in the Local Interstellar Magnetic Field Draped Around Our Heliosphere: Implications for the IBEX Ribbon's Source and IMAP [0.03%]
本地星际磁场包绕我们的日球层时~keV拾取离子的强散射：就IBEX环状带的源和IMAP而言的意义
E J Zirnstein,D J McComas,N A Schwadron et al.
E J Zirnstein et al.
The leading hypothesis for the origin of the Interstellar Boundary Explorer (IBEX) "ribbon" of enhanced energetic neutral atoms (ENAs) from the outer heliosphere is the secondary ENA mechanism, whereby neutralized solar wind ions escape the...
J I Moses,M S Marley,K Zahnle et al.
J I Moses et al.
The past decade has seen significant progress on the direct detection and characterization of young, self-luminous giant planets at wide orbital separations from their host stars. Some of these planets show evidence for disequilibrium proce...
Guillermo Quintana-Lacaci,José Cernicharo,Marcelino Agúndez et al.
Guillermo Quintana-Lacaci et al.
We aim at studying the properties of a particular type of evolved stars, the C-rich evolved stars with high expansion velocities. For this purpose we have focused on the two best studied objects within this group, IRC +10401 and AFGL 2233. ...
ACCRETION OF SATURN'S INNER MID-SIZED MOONS FROM A MASSIVE PRIMORDIAL ICE RING [0.03%]
土卫从一个巨大的原始冰环中聚集形成內部中等大小的卫星簇
J Salmonc,R M Canup
J Salmonc
Saturn's rings are rock-poor, containing 90 to 95% ice by mass. As a group, Saturn's moons interior to and including Tethys are also about 90% ice. Tethys itself contains < 6% rock by mass, in contrast to its similar-mass outer neighbor Dio...
Transition Probabilities of Co ii Weak Lines to the Ground and Low Metastable Levels [0.03%]
Co ii弱线向基态和低激发态转移概率
J E Lawler,T Feigenson,C Sneden et al.
J E Lawler et al.
New branching fraction (BF) measurements based primarily on data from a cross-dispersed echelle spectrometer are reported for 84 lines of Co ii. The BFs for 82 lines are converted to absolute atomic transition probabilities using radiative ...
Triggered Star Formation inside the Shell of a Wolf-Rayet Bubble as the Origin of the Solar System [0.03%]
太阳系形成的启始沃尔夫-拉叶星风泡壳层触发星族形成起源说
Vikram V Dwarkadas,Nicolas Dauphas,Bradley Meyer et al.
Vikram V Dwarkadas et al.
A critical constraint on solar system formation is the high 26Al/27Al abundance ratio of 5 × 10-5 at the time of formation, which was about 17 times higher than the average Galactic ratio, while the 60Fe/56Fe value was about 2 × 10-8, low...
Isotopic Dichotomy among Meteorites and Its Bearing on the Protoplanetary Disk [0.03%]
陨石中的同位素二元性及其对原行星盘的意义
Edward R D Scott,Alexander N Krot,Ian S Sanders
Edward R D Scott
Whole rock Δ17O and nucleosynthetic isotopic variations for chromium, titanium, nickel, and molybdenum in meteorites define two isotopically distinct populations: carbonaceous chondrites (CCs) and some achondrites, pallasites, and irons in...
PROBING THE CARBON-PHOSPHORUS BOND COUPLING IN LOW-TEMPERATURE PHOSPHINE (PH3)-METHANE (CH4) INTERSTELLAR ICE ANALOGUES [0.03%]
低温磷化氢(Ph₃)-甲烷(CH₄)互模拟星际冰中碳磷键偶合的探测研究
Andrew M Turner,Matthew J Abplanalp,Ralf I Kaiser
Andrew M Turner
Phosphine, which has now been confirmed around the carbon-rich star IRC+10216, provides the first example of a phosphorus-containing single bond in interstellar or circumstellar media. While four compounds containing both phosphorus and car...