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CORC

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Broadband Multiwavelength Study of LHAASO-detected Active Galactic Nuclei 期刊论文
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2024, 卷号: 271, 期号: 1
作者:  Wang, Ze-Rui;  Xue, Rui;  Xiong DR(熊定荣);  Wang, Hai-Qin;  Sun, Lu-Ming
收藏  |  浏览/下载：1/0  |  提交时间：2024/03/29
On the Scarcity of Dense Cores (n > 105 cm-3) in High-latitude Planck Galactic Cold Clumps 期刊论文
ASTROPHYSICAL JOURNAL LETTERS, 2024, 卷号: 963, 期号: 1
作者:  Xu, Fengwei;  Wang, Ke;  Liu, Tie;  Eden, David;  Liu, Xunchuan
收藏  |  浏览/下载：1/0  |  提交时间：2024/04/01
Monte Carlo Simulations on Possible Collimation Effects of Outflows to Fan Beam Emission of Ultraluminous Accreting X-Ray Pulsars 期刊论文
ASTROPHYSICAL JOURNAL, 2022, 卷号: 941, 期号: 2
作者:  Hou X(侯贤);  You, Y.;  Ji, L.;  Soria, R.;  Zhang, S. N.
收藏  |  浏览/下载：17/0  |  提交时间：2023/01/16
Fan-beamed X-Ray Emission from 1 to above 130 keV from the Ultraluminous X-Ray Pulsar RX J0209.6-7427 in the Small Magellanic Cloud 期刊论文
ASTROPHYSICAL JOURNAL, 2022, 卷号: 938, 期号: 2
作者:  Hou X(侯贤);  Ge, M. Y.;  Ji, L.;  Zhang, S. N.;  You, Y.
收藏  |  浏览/下载：20/0  |  提交时间：2022/11/07
PDRs4All: A JWST Early Release Science Program on Radiative Feedback from Massive Stars 期刊论文
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 2022, 卷号: 134, 期号: 1035
作者:  Team:, PI;  Berné, Olivier;  Habart, Émilie;  Peeters, Els;  Team:, Core
收藏  |  浏览/下载：23/0  |  提交时间：2022/06/13
Chapter 3 Extra-galactic gamma-ray sources 期刊论文
Chinese Physics C, 2022, 卷号: 46, 期号: 3
作者:  Wang, Xiang-Yu;  Bi, Xiao-Jun;  Cao, Zhen;  Vallania, Piero;  Wu, Han-Rong
收藏  |  浏览/下载：64/0  |  提交时间：2022/03/21
AGN  Gamma-rays  GRBs  
ALCHEMI, an ALMA Comprehensive High-resolution Extragalactic Molecular Inventory Survey presentation and first results from the ACA array 期刊论文
ASTRONOMY & ASTROPHYSICS, 2021, 卷号: 656, 页码: 62
作者:  Martin, S.;  Mangum, J. G.;  Harada, N.;  Costagliola, F.;  Sakamoto, K.
收藏  |  浏览/下载：69/0  |  提交时间：2022/03/21
Starburst Energy Feedback Seen through HCO+/HOC+ Emission in NGC 253 from ALCHEMI 期刊论文
ASTROPHYSICAL JOURNAL, 2021, 卷号: 923, 期号: 1, 页码: 40
作者:  Harada, Nanase;  Martin, Sergio;  Mangum, Jeffrey G.;  Sakamoto, Kazushi;  Muller, Sebastien
收藏  |  浏览/下载：25/0  |  提交时间：2022/03/21
Constraints on a mixed model of dark matter particles and primordial black holes from the galactic 511 keV line 期刊论文
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2021, 期号: 3, 页码: 57
作者:  Cai, Rong-Gen;  Ding, Yu-Chen;  Yang, Xing-Yu;  Zhou, Yu-Feng
收藏  |  浏览/下载：12/0  |  提交时间：2021/09/27
Detection of two bright radio bursts from magnetar SGR 1935 + 2154 期刊论文
Nature Astronomy, 2021, 卷号: 5, 页码: 414
作者:  Kirsten, F.;  Snelders, M. P.;  Jenkins, M.;  Nimmo, K.;  van den Eijnden, J.
收藏  |  浏览/下载：41/0  |  提交时间：2021/11/18
Astrophysics - High Energy Astrophysical Phenomena  Abstract: Fast radio bursts are millisecond-duration, bright radio signals (fluence 0.1-100 Jy ms) emitted from extragalactic sources of unknown physical origin. The recent CHIME/FRB and STARE2 detection of an extremely bright (fluence ~MJy ms) radio burst from the Galactic magnetar SGR 1935+2154 supports the hypothesis that (at least some) fast radio bursts are emitted by magnetars at cosmological distances. In follow-up observations totalling 522.7 h on source, we detect two bright radio bursts with fluences of 112 ± 22 Jy ms and 24 ± 5 Jy ms, respectively. Both bursts appear to be affected by interstellar scattering and we measure significant linear and circular polarization for the fainter burst. The bursts are separated in time by ~1.4 s, suggesting a non-Poissonian, clustered emission processsimilar to those seen in some repeating fast radio bursts. Together with the burst reported by CHIME/FRB and STARE2, as well as a much fainter burst seen by FAST (fluence 60 mJy ms), our observations demonstrate that SGR 1935+2154 can produce bursts with apparent energies spanning roughly seven orders of magnitude, and that the burst rate is comparable across this range. This raises the question of whether these four bursts arise from similar physical processes, and whether the fast radio burst population distribution extends to very low energies (~1030 erg, isotropic equivalent).  

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