WALLABY early science - III. An HI study of the spiral galaxy NGC 1566

This paper reports on the atomic hydrogen gas (H I) observations of the spiral galaxy NGC 1566 using the newly commissioned Australian Square Kilometre Array Pathfinder radio telescope. We measure an integrated H I flux density of 180.2 Jy km s−1 emanating from this galaxy, which translates to an H ...

Täydet tiedot

Bibliografiset tiedot
Päätekijät:	Elagali, A, Staveley-Smith, L, Rhee, J, Wong, O, Bosma, A, Westmeier, T, Koribalski, BS, Heald, G, For, BQ, Kleiner, D, Lee-Waddell, K, Madrid, JP, Popping, A, Reynolds, TN, Meyer, MJ, Allison, JR, Lagos, CDP, Voronkov, MA, Serra, P, Shao, L, Wang, J, Anderson, CS, Bunton, JD, Bekiaris, G, Walsh, VM, Kilborn, VA, Kamphuis, P, Oh, SH
Aineistotyyppi:	Journal article
Kieli:	English
Julkaistu:	Oxford University Press 2019

WALLABY early science - III. An HI study of the spiral galaxy NGC 1566

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