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    ARGO-YBJ: Fruitful Cosmic Ray Observations
    CAO Zhen
    Chinese Journal of Nature    2012, 34 (5): 284-290.  
    Abstract1081)      PDF(pc) (669KB)(1098)       Save
    Being smoothly operated for 5 years, the ARGO-YBJ experiment collected 0.4 trillion cosmic ray event samples. Many scientific goals have been achieved based on the very important data base. Here in this article, we summarize all major contributions to cosmic ray related researches, including conventional measurements such as cosmic ray energy spectrum, composition and anisotropy. The researches also cover many nontraditional topics such as the monitoring of solar activity using Galactic cosmic rays, forecasting large geomagnetic storms induced by huge flares of the sun, exploring the correlation between thunderstorms and extensives air shower of cosmic rays and so forth. With the progresses of the future experiment LHAASO, all researches reported in this paper will be greatly enhanced using the most sensitive new generation apparatus. Breakthrough may be expected in some of the topics. 
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    Barlike structure in the inner Galaxy
    ZHAO Jun-Liang
    Chinese Journal of Nature    2013, 35 (5): 320-325.  
    Abstract885)      PDF(pc) (1043KB)(435)       Save
    The presence of a large scale bar in the inner Galaxy has been well established by various tracers since 1990, such as near infrared radiation (NIR) light, red clump giants, AGB stars and IRAS sources, and by different methods, such as bulge surface brightness, NIR star counts and kinematics of stars. It has been confirmed from various kinds of researches that our Milky Way should be morphologically catalogued as a barred spiral galaxy instead of a normal spiral one.
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    Warp of the outer region of the Galaxy
    ZHAO Jun-Liang
    Chinese Journal of Nature    2013, 35 (6): 396-401.  
    Abstract623)      PDF(pc) (1025KB)(548)       Save
     It is now over 50 years since radio observations of neutral hydrogen revealed the gaseous disk of the Milky Way Galaxy to be warped and flaring. Subsequently, such a structure has also been observed in the distribution of various components of the Galaxy in different wavebands, such as population I objects, molecular clouds, interstellar dust and older star population.
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    Stellar streams and their implication for studies on the structure of our Galaxy
    ZHAO Jun-liang
    Chinese Journal of Nature    2014, 36 (4): 235-240.   DOI: 10.3969/j.issn.0253-9608.2
    Abstract864)      PDF(pc) (1817KB)(1427)       Save
    Many stellar tidal streams in the outer halo of the Milky Way Galaxy have been found since 1994. Some streams are formed from dwarf satellites and others from globular clusters. More and more observational and theoretical studies on the stellar streams have been done during recent 20 years or so, from which some important results were gained.
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    Relativistic baryonic jets from an ultraluminous supersoft X-ray source
    BAI Yu, WANG Song, LIU Jifeng
    Chinese Journal of Nature    2016, 38 (1): 8-14.   DOI: 10.3969/j.issn.0253-9608.2016.01.002
    Abstract1081)      PDF(pc) (4274KB)(1107)       Save
    The formation of relativistic jets by an accreting compact object is one of the fundamental mysteries of astrophysics. While the theory is poorly understood, the observations of relativistic jets from systems known as microquasars have led to a well-established phenomenology. Relativistic jets are not expected from sources with soft or supersoft X-ray spectra, although two such systems are known to produce relatively low-velocity bipolar out?ows. Here we report the optical spectra of an ultraluminous supersoft X-ray source (ULS) in the nearby galaxy M81 (M81 ULS-1) showing blueshifted broad Ha emission lines, the characteristics of baryonic jets with relativistic speeds. The time variable jets have projected velocities ~17 percent of the speed of light, which seems similar to those in the prototype microquasar SS433. Such relativistic jets are not expected to be launched from white dwarfs, but an origin from a black hole or neutron star in M81 ULS-1 is hard to reconcile with its constant soft X-rays. The completely unexpected presence of relativistic jets in a ULS challenges the canonical theories for jet formation, which is possibly explained by a long speculated supercritically accreting black hole with optically thick out?ows.
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    Cited: Baidu(3)
    Gravitational wave and black holes
    ZHANG Tianrong
    Chinese Journal of Nature    2016, 38 (2): 87-93.   DOI: 10.3969/j.issn.0253-9608.2016.02.002
    Abstract906)      PDF(pc) (3038KB)(1619)       Save

    On September 14, 2015, LIGO detected gravitational waves from the merger of two black holes 29 and 36 times the mass of the Sun. This is the first time for human beings to divectly detect such waves and the first observation of a binary black hole merger. What are gravitational waves? What are black holes? How do they connect each other? What happens when black holes collide? Author will explain these for you.

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    Will our sun become a black hole
    ZHANG Tianrong
    Chinese Journal of Nature    2016, 38 (6): 456-460.   DOI: 10.3969/j.issn.0253-9608.2016.06.009
    Abstract835)      PDF(pc) (1196KB)(2137)       Save

    Will our sun become a black hole? No. Stars like the Sun just are not massive enough to become black hole. Instead, in several billion years, the Sun will cast off its outer layer, and its core will form a white dwarf, a dense ball of carbon and oxygen that no longer produces nuclear energy, which still shines because it is very hot. A typical white dwarf is about as massive as the Sun, but only as big as the Earth, which is one percent of the Sun’s present diameter.

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    The puzzle of black hole information loss
    HE Dongshan, CAI Qingyu
    Chinese Journal of Nature    2018, 40 (4): 242-244.   DOI: 10.3969/j.issn.0253-9608.2018.04.002
    Abstract914)      PDF(pc) (771KB)(676)       Save

    Unitarity is required by quantum mechanics for the dynamics of any closed systems, i.e., information is conserved for closed systems. The black hole information loss conflicts to the unitarity, which indicates the impossibility of unifying quantum mechanics with gravity. In this paper, we review the origin of the puzzle and the possible solutions.

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    The first black hole image: An introduction to black hole
    WU Qingwen
    Chinese Journal of Nature    2019, 41 (3): 157-167.   DOI: 10.3969/j.issn.0253-9608.2019.03.001
    Abstract1347)      PDF(pc) (8662KB)(1935)       Save
    Einstein discovered the special relativity and general relativity at 1905 and 1915 respectively. The most fundamental prediction of the general relativity is the existence of black hole. Now, we believe that there is a supermassive black hole and possibly billion of stellar-mass black holes in each galaxy. It is still unclear whether the intermediate mass of black hole exist or not. There are many indirect evidences for the existence of black holes at different scales by measuring the effects of an object surrounding the black
    holes. The international collaboration group for the event horizon telescope try to achieve the high resolution that can resolve the
    horizon of the two nearby supermassive black holes (in Milky Way and M87 at the center of Virgo cluster) by adopting a technique
    known as very-long-baseline interferometry. For about 10 days in April of 2017, the scientists observed the Sgr A* and M87 by networking eight telescopes around the globe. In April 10 of 2019, the group of the event horizon telescope announced the first photo of the black hole at the center of M87, which is the most direct evidence for the existence of the black hole. This results further support the theory of the general relativity. In last part, I also simply review the possible future Chinese projects that will focus on the black hole physics.
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    Black hole marks a new era of muti-messenger astronomy
    LI Cong
    Chinese Journal of Nature    2019, 41 (3): 219-223.   DOI: 10.3969/j.issn.0253-9608.2019.03.008
    Abstract1339)      PDF(pc) (4294KB)(601)       Save
    Black hole is the most mysterious object in the universe, which has only existed in the theoretical hypothesis for a long time. However, with the development of modern astronomy, we have got many evidences for existence of black hole. Especially with
    the development of gravitational wave and neutrino detection, we can not only get information from black hole via electromagnetic
    radiation but other “messengers”, which marks a new era of muti-messenger astronomy!
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    Black hole information paradox: Is the information that fell into the black hole lost?
    YU Minghui, GE Xianhui
    Chinese Journal of Nature    2021, 43 (2): 127-134.   DOI: 10.3969/j.issn.0253-9608.2021.02.007
    Abstract1112)      PDF(pc) (3808KB)(1664)       Save
    The black hole information paradox has bedeviled theoretical physicists for nearly 50 years since it was entranced. It is regarded as an important approach to study the theory of quantum gravity. The key to the question is whether the Page curve of the black hole evaporation process can be given. However, in the last year, the research of this problem was made a breakthrough. Physicists calculated the Page curve under the semiclassical theory of gravity, showing that information was indeed released during the evaporation of the black hole and no information was lost. This also announces the solution of the black hole information problem. This paper introduces the history and latest progress of the research on black hole information paradox in chronological order. 
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    Interpret the latest parameter measurement results of Cygnus X-1
    ZHAO Xueshan, FENG Ye, GOU Lijun
    Chinese Journal of Nature    2021, 43 (3): 209-216.   DOI: 10.3969/j.issn.0253-9608.2021.03.006
    Abstract1166)      PDF(pc) (3053KB)(930)       Save
    Cygnus X-1 discovered in 1964 was the first stellar mass black hole that has ever been observed, which continues to fascinate astronomers. Accurate measurements of the systematical parameters will help astronomers better understand its physical properties and put better limits on the evolution of stars. In 2011, the mass, distance, spin and other parameters of this system were comprehensive measured for the first time. In 2021, an international team including researchers from NAOC again made precise measurements and updated all the systematical parameters of Cygnus X-1. In this paper, we introduce the methods for measuring the mass, distance and spin of Cygnus X-1, present results of two previous precise measurements made in 2011 and 2021, respectively, and discuss the implications of the latest measurements on the stellar and binary evolution.
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    Measurements of the solar magnetic fields
    LI Wenxian, TIAN Hui
    Chinese Journal of Nature    2022, 44 (1): 19-30.   DOI: 10.3969/j.issn.0253-9608.2022.01.002
    Abstract1288)      PDF(pc) (7031KB)(2263)       Save
    The discovery of magnetic field in sunspots in 1908 brought solar physics from phenomenological observations to studies on the basis of physics. The solar magnetic field couples the solar interior with the visible surface of the Sun and with its entire atmosphere. Evolution of the solar magnetic field drives various types of activity in the solar atmosphere. The accurate measurement of solar magnetic fields is critical to our understanding of most unsolved problems in solar physics. In this article, we give an overview of the solar magnetic field measurements, including Hale’s discovery, history of solar magnetic field observations, and various methods for magnetic field measurements. The challenges and prospects for future research are also discussed.
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