Planck data towards the galaxy M 82 are analyzed in the 70, 100 and 143 GHz bands. A substantial north-south and east-west temperature asymmetry is found, extending up to 1° from the galactic center. Being almost frequency-independent, these temperature asymmetries are indicative of a Doppler-induced effect regarding the line-of-sight dynamics on the halo scale, the ejections from the galactic center and, possibly, even the tidal interaction with M 81 galaxy. The temperature asymmetry thus acts as a model-independent tool to reveal the bulk dynamics in nearby edge-on spiral galaxies, like the Sunyaev-Zeldovich effect for clusters of galaxies.
Planck view of the M 82 galaxy / Gurzadyan, V. G.; De Paolis, F.; Nucita, A. A.; Ingrosso, G.; Kashin, A. L.; Khachatryan, H. G.; Sargsyan, S.; Yegorian, G.; Jetzer, Ph.; Qadir, A.; Vetrugno, D.. - In: ASTRONOMY & ASTROPHYSICS. - ISSN 0004-6361. - 582:(2015), p. A77. [10.1051/0004-6361/201527132]
Planck view of the M 82 galaxy
Vetrugno D.
2015-01-01
Abstract
Planck data towards the galaxy M 82 are analyzed in the 70, 100 and 143 GHz bands. A substantial north-south and east-west temperature asymmetry is found, extending up to 1° from the galactic center. Being almost frequency-independent, these temperature asymmetries are indicative of a Doppler-induced effect regarding the line-of-sight dynamics on the halo scale, the ejections from the galactic center and, possibly, even the tidal interaction with M 81 galaxy. The temperature asymmetry thus acts as a model-independent tool to reveal the bulk dynamics in nearby edge-on spiral galaxies, like the Sunyaev-Zeldovich effect for clusters of galaxies.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione
