Inflation of 430-parsec bipolar radio bubbles in the Galactic Centre by an energetic event

The Galactic Centre contains a supermassive black hole with a mass of four million Suns1 within an environment that differs markedly from that of the Galactic disk. Although the black hole is essentially quiescent in the broader context of active galactic nuclei, X-ray observations have provided evi...

Täydet tiedot

Bibliografiset tiedot
Päätekijät: Heywood, I, Camilo, F, Cotton, WD, Yusef-Zadeh, F, Abbott, TD, Adam, RM, Aldera, MA, Bauermeister, EF, Booth, RS, Botha, AG, Botha, DH, Brederode, LRS, Brits, ZB, Buchner, SJ, Burger, JP, Chalmers. JM, Cheetham, T, de Villiers, D, Dikgale-Mahlakoana, MA, du Toit, LJ, Esterhuyse, SWP, Fanaroff, BL, Foley, AR, Fourie, DJ, Gamatham, RRG, Goedhart, S, Gounden, S, Hlakola, MJ, Hoek, CJ, Hokwana, A, Horn, DM, Horrell, JMG, Hugo, B, Isaacson, AR, Jonas, JL, Jordaan, JDBL, Joubert, AF, Józsa, GIG, Julie, RPM, Kap, FB, Kenyon, JS, Kotzé, PPA, Kriel, H, Kusel, TW, Lehmensiek, R, Liebenberg, D, Loots, A, Lord, RT, Lunsky, BM, Macfarlane, PS
Aineistotyyppi: Journal article
Kieli:English
Julkaistu: Nature Research 2019
Aiheet: