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Items: 4

1.

A rapidly changing jet orientation in the stellar-mass black-hole system V404 Cygni.

Miller-Jones JCA, Tetarenko AJ, Sivakoff GR, Middleton MJ, Altamirano D, Anderson GE, Belloni TM, Fender RP, Jonker PG, Körding EG, Krimm HA, Maitra D, Markoff S, Migliari S, Mooley KP, Rupen MP, Russell DM, Russell TD, Sarazin CL, Soria R, Tudose V.

Nature. 2019 May;569(7756):374-377. doi: 10.1038/s41586-019-1152-0. Epub 2019 Apr 29.

PMID:
31036949
2.

Accretion-induced variability links young stellar objects, white dwarfs, and black holes.

Scaringi S, Maccarone TJ, Körding E, Knigge C, Vaughan S, Marsh TR, Aranzana E, Dhillon VS, Barros SC.

Sci Adv. 2015 Oct 9;1(9):e1500686. doi: 10.1126/sciadv.1500686. eCollection 2015 Oct.

3.

An accurate geometric distance to the compact binary SS Cygni vindicates accretion disc theory.

Miller-Jones JC, Sivakoff GR, Knigge C, Körding EG, Templeton M, Waagen EO.

Science. 2013 May 24;340(6135):950-2. doi: 10.1126/science.1237145.

4.

A transient radio jet in an erupting dwarf nova.

Körding E, Rupen M, Knigge C, Fender R, Dhawan V, Templeton M, Muxlow T.

Science. 2008 Jun 6;320(5881):1318-20. doi: 10.1126/science.1155492.

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