Nature Search

A new class of extragalactic radio sources with one-sided structure?

D. J. Saikia
W. Junor
A. K. Tzioumis
Research25 May 1989
Nature

Volume: 339, P: 286-288
Structure of the radio remnant of supernova 1987A

L. Staveley-Smith
D. S. Briggs
M. J. Kesteven
Research11 Nov 1993
Nature

Volume: 366, P: 136-138
Birth of a radio supernova remnant in supernova 1987A

L. Staveley-Smfth
R. N. Manchester
D. L. Jauncey
Research09 Jan 1992
Nature

Volume: 355, P: 147-149
A disrupted radio jet inside the host galaxy of the quasar 3C48

P. N. Wilkinson
A. K. Tzioumis
F. D. Kahn
Research25 Jul 1991
Nature

Volume: 352, P: 313-315
An unusually strong Einstein ring in the radio source PKS1830–211

D. L. Jauncey
J. E. Reynolds
G. L. White
Research11 Jul 1991
Nature

Volume: 352, P: 132-134
A planet orbiting the neutron star PSR1829–10

M. Bailes
A. G. Lyne
S. L. Shemar
Research25 Jul 1991
Nature

Volume: 352, P: 311-313
Relativistic motion in a nearby bright X-ray source

S. J. Tingay
D. L. Jauncey
D. Smits
Research09 Mar 1995
Nature

Volume: 374, P: 141-143
Financial constraints and firms’ markup: evidence from China

Wen Yue
Xuefei Li
ResearchOpen Access04 Apr 2023
Humanities and Social Sciences Communications

Volume: 10, P: 1-13
Coincidence of a high-fluence blazar outburst with a PeV-energy neutrino event

The IceCube neutrino telescope in the South Pole has observed several high-energy neutrinos of undetermined origin. Could the third detected PeV event be from blazar PKS B1424–418?

M. Kadler
F. Krauß
J. A. Zensus
Research18 Apr 2016
Nature Physics

Volume: 12, P: 807-814
Nine-hour X-ray quasi-periodic eruptions from a low-mass black hole galactic nucleus

Galaxy GSN 069 has unprecedented eruptions of X-ray light every nine hours, which indicate fast transitions between cold and warm states and may shed light on black hole accretion.

G. Miniutti
R. D. Saxton
B. Agís-González
Research11 Sept 2019
Nature

Volume: 573, P: 381-384
Baryons in the relativistic jets of the stellar-mass black-hole candidate 4U 1630-47

Doppler-shifted X-ray emission lines from highly-ionized atoms, appearing together with radio emission from the relativistic jets of the black-hole candidate X-ray binary 4U 1630-47, indicate that the X-ray emission lines arise in a jet travelling at approximately two-thirds the speed of light and imply that the jet contains baryons.

María Díaz Trigo
James C. A. Miller-Jones
Tasso Tzioumis
Research13 Nov 2013
Nature

Volume: 504, P: 260-262

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