搜索结果: 1-6 共查到“天文学 Revealing”相关记录6条 . 查询时间(0.063 秒)
Revealing the Recycled inflow of the massive galaxies at high redshift
high redshift massive galaxies Recycled inflow
font style='font-size:12px;'>
2023/6/19
The gas surrounding galaxies is known as the circumgalactic medium (CGM) which is considered to be deeply coupled with the evolution of galaxies. Although lots of works have been done, how galaxies co...
"Revealing a Population of Heavily Obscured Active Galactic Nuclei at z=0.5-1 in the Chandra Deep Field-South
Revealing Population Heavily Obscured Active Galactic Nuclei
font style='font-size:12px;'>
2011/10/10
We identify a numerically significant population of heavily obscured AGNs at z~0.5-1 in the Chandra Deep Field-South (CDF-S) and Extended Chandra Deep Field-South by selecting 242 X-ray undetected obj...
Revealing the physics of r-modes in low-mass X-ray binaries
Revealing the physics of r-modes in low-mass X-ray binaries
font style='font-size:12px;'>
2011/10/21
We consider the astrophysical constraints on the gravitational-wave driven r-mode instability in accreting neutron stars in low-mass X-ray binaries. We use recent results on superfluid and superconduc...
Evolution of Infrared Luminosity functions of Galaxies in the AKARI NEP-Deep field: Revealing the cosmic star formation history hidden by dust
galaxies evolution galaxies interactions galaxies:starburst galaxies peculiar galaxies formation
font style='font-size:12px;'>
2010/3/8
Dust-obscured star-formation becomes much more important with increasing intensity, and increasing redshift. We aim to reveal cosmic star-formation history obscured by dust using deep infrared observa...
Revealing the nature of the highly obscured galactic Source igr j16318-4848
highly obscured galactic Source igr j16318-4848
font style='font-size:12px;'>
2009/6/17
Revealing the nature of the highly obscured galactic Source igr j16318-4848。
Revealing the physical changes taking place in z-track Motion in low mass x-ray binaries
z-track Motion low mass x-ray binaries
font style='font-size:12px;'>
2009/6/17
Revealing the physical changes taking place in z-track Motion in low mass x-ray binaries。