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Young galaxies blaze with bright new stars forming at a rapid rate, but star formation eventually shuts down as a galaxy evolves. A new study, published January 1, 2018, in Nature, shows that the mass...
Three months of observations with the National Science Foundation’s Karl G. Jansky Very Large Array (VLA) have allowed astronomers to zero in on the most likely explanation for what happened in the af...
Radio “Eyes” Unlocking Secrets of Neutron-Star Collision(图)     Radio  Eyes  Unlocking  Neutron-Star Collision       font style='font-size:12px;'> 2017/10/26
When a pair of superdense neutron stars collided and potentially formed a black hole in a galaxy 130 million light-years from Earth, they unleashed not only a train of gravitational waves but also an ...
A University of Oklahoma astrophysicist, Mukremin Kilic, and his team have discovered two detached, eclipsing double white dwarf binaries with orbital periods of 40 and 46 minutes, respectively. White...
STAR国际合作组首次测量到超子的整体极化效应     STAR  超子  整体极化效应       font style='font-size:12px;'> 2017/8/23
最近,由中国科学技术大学学者在内的中国科学家参加的美国布鲁克海文国家实验室STAR国际合作组在重离子碰撞中首次观测到了夸克胶子等离子体(QGP)的“整体极化”(global polarization),发现碰撞产生的Lambda超子相对于碰撞反应平面存在明显的自旋极化。STAR国际合作组的该研究成果于8月3日作为封面文章发表在《自然》杂志上【Nature 548, 62-65 (2017)】。在这...
An ancient, red giant star in the throes of a frigid death has produced the coldest known object in the cosmos — the Boomerang Nebula. How this star was able to create an environment strikingly colder...
Gemini Tracks Distant Star Cluster with Adaptive Optics     Gemini  Distant Star Cluster  Adaptive Optics       font style='font-size:12px;'> 2017/7/20
We present a proper motion measurement for the halo globular cluster Pyxis, using HST/ACS data as the first epoch, and GeMS/GSAOI Adaptive Optics data as the second, separated by a baseline of ~ 5 yea...
Dormant Black Hole Eats Star,Becomes X-Ray Beacon     Dormant Black Hole  Eats Star  X-Ray Beacon       font style='font-size:12px;'> 2016/7/4
Roughly 90 percent of the biggest black holes in the known universe are dormant, meaning that they are not actively devouring matter and, consequently, not giving off any light or other radiation. But...
Cool,Dim Dwarf Star is Magnetic Powerhouse     Cool  Dim Dwarf Star  Magnetic Powerhouse       font style='font-size:12px;'> 2015/12/7
Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA)have discovered that a dim, cool dwarf star is generating a surprisingly powerful magnetic field, one that rivals the most...
Globular clusters – dazzling agglomerations of up to a million ancient stars – are among the oldest objects in the universe. Though plentiful in and around many galaxies, newborn examples are vanishin...
The number of known Be/X-ray binaries in the Large Magellanic Cloud is small compared to the observed population of the Galaxy or the Small Magellanic Cloud. The discovery of a system in outburst prov...
Abridged: Four new nuclear star cluster masses, M_nc, plus seven upper limits, are provided for galaxies with previously determined black hole masses, M_bh. Together with a sample of 64 galaxies with ...
Low-mass X-ray binaries (LMXBs) are systems in which a low-mass companion transfers mass via Roche-lobe overflow onto a black hole (BH) or a weakly magnetized neutron star (NS). It is believed that bo...
Massive-Star Nucleosynthesis and INTEGRAL     Massive-Star Nucleosynthesis  INTEGRAL       font style='font-size:12px;'> 2011/10/19
Products from massive-star nucleosynthesis have been measured with SPI on INTEGRAL: Characteristic gamma-ray lines from radioactive decays of long-lived 26Al and 60Fe isotopes, and from 44Ti decay (de...
We study the spectrum of collective excitations in the inhomogeneous phases in the neutron star inner crust within a superfluid hydrodynamics approach. Our aim is to describe the whole range of wavele...

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