The power of relativistic jets is larger than the luminosity of their accretion disks.
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SDSS J013127.34–032100.1: a candidate blazar with an 11 billion solar mass black hole at z = 5.18The puzzling case of the radio-loud QSO 3C 186: a gravitational wave recoiling black hole in a young radio source?First-generation science cases for ground-based terahertz telescopesA significant hardening and rising shape detected in the MeV/GeV νFνspectrum from the recently discovered very-high-energy blazar S4 0954+65 during the bright optical flare in 2015 FebruaryA simplified view of blazars: the neutrino backgroundCMB quenching of high-redshift radio-loud AGNsHigh-energy cosmic neutrinos from spine-sheath BL Lac jetsFermi/LAT broad emission line blazarsA newly discovered double-double candidate microquasar in NGC 300
P2860
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P2860
The power of relativistic jets is larger than the luminosity of their accretion disks.
description
2014 nî lūn-bûn
@nan
2014年の論文
@ja
2014年論文
@yue
2014年論文
@zh-hant
2014年論文
@zh-hk
2014年論文
@zh-mo
2014年論文
@zh-tw
2014年论文
@wuu
2014年论文
@zh
2014年论文
@zh-cn
name
The power of relativistic jets is larger than the luminosity of their accretion disks.
@en
type
label
The power of relativistic jets is larger than the luminosity of their accretion disks.
@en
prefLabel
The power of relativistic jets is larger than the luminosity of their accretion disks.
@en
P50
P356
P1433
P1476
The power of relativistic jets is larger than the luminosity of their accretion disks.
@en
P2093
P2888
P304
P356
10.1038/NATURE13856
P407
P577
2014-11-01T00:00:00Z
P5875
P6179
1040905740
P698
P818
P819
2014Natur.515..376G