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
We used Planck data to study the M 33 galaxy and find a substantial temperature asymmetry with respe...
Data on the cosmic microwave background (CMB) radiation by the Wilkinson Microwave Anisotr...
We perform an analysis of the CMB temperature data taken by the Planck satellite investigating if th...
Planck data towards the galaxy M 82 are analyzed in the 70, 100 and 143 GHz bands. A substantial nor...
Planck data towards the galaxy M82 are analyzed in the 70, 100 and 143 GHz bands. A substantial nort...
Planck data acquired during the first 15.4 months of observations toward both the disk and halo of t...
This paper is a follow-up of a previous paper about the M 82 galaxy and its halo based on Planck obs...
This paper is a follow-up of a previous paper about the M 82 galaxy and its halo based on Planck obs...
Planck's data acquired during the first 15.4 months of observations towards both the disk and halo o...
Planck data acquired during the first 15.4 months of observations toward both the disk and halo of t...
Planck data towards the active galaxy Centaurus A are analyzed in the 70, 100 and 143 GHz bands. We ...
Galactic halos are of great importance for our understanding of both the dark matter nature and prim...
Planck data towards the active galaxy Centaurus A are analyzed in the 70, 100 and 143 GHz bands. We ...
Temperature asymmetry in the cosmic microwave background (CMB) data by the Planck satellite has been...
We used Planck data to study the M 33 galaxy and find a substantial temperature asymmetry with respe...
We used Planck data to study the M 33 galaxy and find a substantial temperature asymmetry with respe...
Data on the cosmic microwave background (CMB) radiation by the Wilkinson Microwave Anisotr...
We perform an analysis of the CMB temperature data taken by the Planck satellite investigating if th...
Planck data towards the galaxy M 82 are analyzed in the 70, 100 and 143 GHz bands. A substantial nor...
Planck data towards the galaxy M82 are analyzed in the 70, 100 and 143 GHz bands. A substantial nort...
Planck data acquired during the first 15.4 months of observations toward both the disk and halo of t...
This paper is a follow-up of a previous paper about the M 82 galaxy and its halo based on Planck obs...
This paper is a follow-up of a previous paper about the M 82 galaxy and its halo based on Planck obs...
Planck's data acquired during the first 15.4 months of observations towards both the disk and halo o...
Planck data acquired during the first 15.4 months of observations toward both the disk and halo of t...
Planck data towards the active galaxy Centaurus A are analyzed in the 70, 100 and 143 GHz bands. We ...
Galactic halos are of great importance for our understanding of both the dark matter nature and prim...
Planck data towards the active galaxy Centaurus A are analyzed in the 70, 100 and 143 GHz bands. We ...
Temperature asymmetry in the cosmic microwave background (CMB) data by the Planck satellite has been...
We used Planck data to study the M 33 galaxy and find a substantial temperature asymmetry with respe...
We used Planck data to study the M 33 galaxy and find a substantial temperature asymmetry with respe...
Data on the cosmic microwave background (CMB) radiation by the Wilkinson Microwave Anisotr...
We perform an analysis of the CMB temperature data taken by the Planck satellite investigating if th...