High Energy Astrophysics Science Archive Research Center (HEASARC)
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the High Energy Astrophysics Science Archive Research Center

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High Energy Astrophysics Science Archive Research Center (HEASARC)

The High Energy Astrophysics Science Archive Research Center (HEASARC) is the primary archive for NASA’s (and other space agencies’) missions studying electromagnetic radiation from extremely energetic cosmic phenomena ranging from black holes to the Big Bang. Since its merger with the Legacy Archive for Microwave Background Data Analysis (LAMBDA) in 2008, the HEASARC archive contains data obtained by high-energy astronomy missions observing in the extreme-ultraviolet (EUV), X-ray, and gamma-ray bands, as well as data from space missions, balloons, and ground-based facilities that have studied the relic cosmic microwave background (CMB) radiation in the sub-mm, mm and cm bands.

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相关论文

13

Cygnus X-3 revealed as a Galactic ultraluminous X-ray source by IXPE

Alexandra VeledinaFabio MuleriJuri PoutanenJakub PodgornýMichal Dovčiak130
Nature Astronomy
2024
2024/6/21
00 p.1-16
The accretion of matter by compact objects can be inhibited by radiation pressure if the luminosity exceeds a critical value known as the Eddington limit. The discovery of ultraluminous X-ray sources has shown that accretion can proceed even when the apparent luminosity considerably exceeds this lim...
Compact astrophysical objectsHigh-energy astrophysics
10.1038/S41550-024-02294-9
ISSN:2397-3366

Structured ionized winds shooting out from a quasar at relativistic speeds

Nature
2025
2025/5/14
00 p.1-5
Evidence indicates that supermassive black holes (SMBHs) exist at the centres of most galaxies. Their mass correlates with the galactic bulge mass1, suggesting a coevolution with their host galaxies2, most likely through powerful winds3. X-ray observations have detected highly ionized winds outflowi...
Compact astrophysical objectsHigh-energy astrophysics
10.1038/S41586-025-08968-2
ISSN:0028-0836

Accurate determination of chemical abundances near a supermassive black hole

Nature Astronomy
2026
2026/3/31
00 p.1-12
The metal abundances in galactic nuclei carry key information on the history of star formation and mass transfer in central regions of galaxies. X-ray fluorescence analysis is a unique tool to reliably measure the abundances of various elements via simple physics. Here we present a new observation o...
Compact astrophysical objectsHigh-energy astrophysics
10.1038/S41550-026-02817-6
ISSN:2397-3366

Determination of X-ray pulsar geometry with IXPE polarimetry

Doroshenko VictorPoutanen JuriTsygankov Sergey S.Suleimanov Valery F.Bachetti Matteo94
Nature Astronomy
2022
2022/10/24
Vol.6 No.12 p.1433-1443
Using observations of X-ray pulsar Hercules X-1 by the Imaging X-ray Polarimetry Explorer we report a highly significant (>17σ) detection of the polarization signal from an accreting neutron star. The observed degree of linear polarization of ~10% is far below theoretical expectations for this ob...
Compact astrophysical objectsHigh-energy astrophysics
10.1038/S41550-022-01799-5
ISSN:2397-3366

A nearby long gamma-ray burst from a merger of compact objects

Troja E.Fryer C. L.O’Connor B.Ryan G.Dichiara S.24
Nature
2022
2022/12/7
Vol.612 No.7939 p.228-231
Gamma-ray bursts (GRBs) are flashes of high-energy radiation arising from energetic cosmic explosions. Bursts of long (greater than two seconds) duration are produced by the core-collapse of massive stars1, and those of short (less than two seconds) duration by the merger of compact objects, such as...
Compact astrophysical objectsHigh-energy astrophysics
10.1038/S41586-022-05327-3
ISSN:0028-0836

Light bending and X-ray echoes from behind a supermassive black hole

Wilkins D. R.Gallo L. C.Costantini E.Brandt W. N.Blandford R. D.
Nature
2021
2021/7/28
Vol.595 No.7869 p.657-660
The innermost regions of accretion disks around black holes are strongly irradiated by X-rays that are emitted from a highly variable, compact corona, in the immediate vicinity of the black hole1–3. The X-rays that are seen reflected from the disk4, and the time delays, as variations in the X-ray em...
Compact astrophysical objectsGeneral relativity and gravityHigh-energy astrophysics
10.1038/S41586-021-03667-0
ISSN:0028-0836

Coupling between the accreting corona and the relativistic jet in the microquasar GRS 1915+105

Méndez MarianoKarpouzas KonstantinosGarcía FedericoZhang LiangZhang Yuexin7
Nature Astronomy
2022
2022/3/7
00 p.1-7
Accreting black holes emit highly collimated radio jets expanding at speeds approaching light speed. Some of these jets appear to be expanding at superluminal speeds due to geometric effects. While magnetic fields are thought to be responsible for collimating the ejecta, the mechanism that accelerat...
Compact astrophysical objectsHigh-energy astrophysics
10.1038/S41550-022-01617-Y
ISSN:2397-3366

Observation and origin of non-thermal hard X-rays from Jupiter

Mori KayaHailey CharlesBridges GabrielMandel ShifraGarvin Amani13
Nature Astronomy
2022
2022/2/10
00 p.1-7
Electrons accelerated on Earth by a rich variety of wave-scattering or stochastic processes1,2 generate hard, non-thermal X-ray bremsstrahlung up to ~1 MeV (refs. 3,4) and power Earth’s various types of aurorae. Although Jupiter’s magnetic field is an order of magnitude larger than Earth’s, space-ba...
Giant planetsHigh-energy astrophysics
10.1038/S41550-021-01594-8
ISSN:2397-3366

Vela pulsar wind nebula X-rays are polarized to near the synchrotron limit

Xie FeiDi Marco AlessandroLa Monaca FabioLiu KuanMuleri Fabio93
Nature
2022
2022/12/21
Vol.612 No.7941 p.658-660
Pulsar wind nebulae are formed when outflows of relativistic electrons and positrons hit the surrounding supernova remnant or interstellar medium at a shock front. The Vela pulsar wind nebula is powered by a young pulsar (B0833-45, aged 11,000 years)1 and located inside an extended structure called ...
High-energy astrophysicsParticle astrophysics
10.1038/S41586-022-05476-5
ISSN:0028-0836

Diffuse X-ray emission around an ultraluminous X-ray pulsar

Andrea BelfiorePaolo EspositoFabio PintoreGiovanni NovaraRuben Salvaterra20
Nature Astronomy
2019
2019/10/28
Vol.4 No.2 p.147-152
Ultraluminous X-ray sources (ULXs) are extragalactic X-ray emitters located off-centre of their host galaxy and with a luminosity in excess of a few 1039 erg s−1, if emitted isotropically1,2. The discovery of periodic modulation revealed that in some ULXs the accreting compact object is a neutron st...
Compact astrophysical objectsHigh-energy astrophysics
10.1038/S41550-019-0903-Z
ISSN:2397-3366

The corona contracts in a black-hole transient

E. KaraJ. F. SteinerA. C. FabianE. M. CackettP. Uttley14
Nature
2019
2019/1/9
Vol.565 No.7738 p.198-201
The geometry of the accretion flow around stellar-mass black holes can change on timescales of days to months1–3. When a black hole emerges from quiescence (that is, it ‘turns on’ after accreting material from its companion) it has a very hard (high-energy) X-ray spectrum produced by a hot corona4,5...
High-energy astrophysicsTransient astrophysical phenomena
10.1038/S41586-018-0803-X
ISSN:0028-0836

Vigorous turbulence driven by quasar-mode feedback in a cluster core

Satoshi YamadaShutaro UedaHirofumi NodaYutaka FujitaMisaki Mizumoto12
Nature Astronomy
2026
2026/7/28
00 p.1-8
Quasars are among the most luminous objects. They are powered by accretion onto supermassive black holes. They are thought to impact cosmological evolution primarily through energetic winds, known as quasar-mode feedback, yet the efficiency and spatial extent of this process remain poorly constraine...
Compact astrophysical objectsCosmologyEarly universeGalaxies and clustersHigh-energy astrophysics
10.1038/S41550-026-02939-X
ISSN:2397-3366

Suppressed effective viscosity in the bulk intergalactic plasma

I. ZhuravlevaE. ChurazovA. A. SchekochihinS. W. AllenA. Vikhlinin6
Nature Astronomy
2019
2019/6/17
Vol.3 No.9 p.832-837
Transport properties, such as viscosity and thermal conduction, of the hot intergalactic plasma in clusters of galaxies are largely unknown. Whereas for laboratory plasmas these characteristics are derived from the gas density and temperature1, such recipes can be fundamentally different for the int...
Astronomy and astrophysicsAstronomy and planetary scienceHigh-energy astrophysics
10.1038/S41550-019-0794-Z
ISSN:2397-3366