Connecting X-ray absorption and 21 cm neutral hydrogen absorption in obscured radio AGN

Many radio galaxies show the presence of dense and dusty gas near the active nucleus. This can be traced by both 21 cm H I absorption and soft X-ray absorption, offering new insight into the physical nature of the circumnuclear medium of these distant galaxies. To better understand this relationship...

Täydet tiedot

Bibliografiset tiedot
Päätekijät:	Moss, VA, Allison, JR, Sadler, EM, Urquhart, R, Soria, R, Callingham, JR, Curran, SJ, Musaeva, A, Mahony, EK, Glowacki, M, Farrell, SA, Bannister, KW, Chippendale, AP, Edwards, PG, Harvey-Smith, L, Heywood, I, Hotan, AW, Indermuehle, BT, Lenc, E, Marvil, J, McConnell, D, Reynolds, JE, Voronkov, MA, Wark, RM, Whiting, MT
Aineistotyyppi:	Journal article
Julkaistu:	Oxford University Press 2017

Connecting X-ray absorption and 21 cm neutral hydrogen absorption in obscured radio AGN

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