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Triangulum galaxy viewed byPlanck


De Paolis, F; Gurzadyan, V. G; Nucita, A. A; Chemin, L; Qadir, A; Kashin, A. L; Khachatryan, H. G; Sargsyan, S; Yegorian, G; Ingrosso, G; Jetzer, Ph; Vetrugno, D (2016). Triangulum galaxy viewed byPlanck. Astronomy and Astrophysics, 593:A57.

Abstract

We used Planck data to study the M 33 galaxy and find a substantial temperature asymmetry with respect to its minor axis projected onto the sky plane. This temperature asymmetry correlates well with the HI velocity field at 21 cm, at least within a galactocentric distance of 0.5°, and it is found to extend up to about 3° from the galaxy center. We conclude that the revealed effect, that is, the temperature asymmetry and its extension, implies that we detected the differential rotation of the M 33 galaxy and of its extended baryonic halo.

Abstract

We used Planck data to study the M 33 galaxy and find a substantial temperature asymmetry with respect to its minor axis projected onto the sky plane. This temperature asymmetry correlates well with the HI velocity field at 21 cm, at least within a galactocentric distance of 0.5°, and it is found to extend up to about 3° from the galaxy center. We conclude that the revealed effect, that is, the temperature asymmetry and its extension, implies that we detected the differential rotation of the M 33 galaxy and of its extended baryonic halo.

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Additional indexing

Item Type:Journal Article, refereed, original work
Communities & Collections:07 Faculty of Science > Physics Institute
Dewey Decimal Classification:530 Physics
Date:2016
Deposited On:29 Dec 2016 10:40
Last Modified:02 Feb 2018 11:10
Publisher:EDP Sciences
ISSN:0004-6361
OA Status:Closed
Free access at:Publisher DOI. An embargo period may apply.
Publisher DOI:https://doi.org/10.1051/0004-6361/201628780

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