Planck confirmation of the disk and halo rotation of M 31

被引:28
作者
De Paolis, F. [1 ,2 ]
Gurzadyan, V. G. [3 ,4 ]
Nucita, A. A. [1 ,2 ]
Ingrosso, G. [1 ,2 ]
Kashin, A. L. [3 ,4 ]
Khachatryan, H. G. [3 ,4 ]
Mirzoyan, S. [3 ,4 ]
Poghosian, E. [3 ,4 ]
Jetzer, Ph [5 ]
Qadir, A. [6 ]
Vetrugno, D. [7 ,8 ]
机构
[1] Univ Salento, Dipartimento Matemat & Fis E De Giorgi, I-73100 Lecce, Italy
[2] Ist Nazl Fis Nucl, Sez Lecce, I-73100 Lecce, Italy
[3] Yerevan Phys Inst, Yerevan 375049, Armenia
[4] Yerevan State Univ, Yerevan 375049, Armenia
[5] Univ Zurich, Phys Inst, CH-8057 Zurich, Switzerland
[6] Natl Univ Sci & Technol, Ctr Adv Math & Phys, Rawalpindi 46000, Pakistan
[7] Univ Trento, Dept Phys, I-38123 Povo, Italy
[8] Ist Nazl Fis Nucl, TIFPA, I-38123 Povo, Italy
基金
瑞士国家科学基金会;
关键词
galaxies: general; galaxies: individual: M 31; galaxies: halos; KINEMATICS; GALAXY;
D O I
10.1051/0004-6361/201423849
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Planck data acquired during the first 15.4 months of observations toward both the disk and halo of the M 31 galaxy were analyzed. We confirm the temperature asymmetry that was previously detected by using the seven-year WMAP data in the direction of the rotation of M 31, which indicates that this is a Doppler-induced effect. The asymmetry extends to about 10 degrees (similar or equal to 130 kpc) from the center of M 31. We also investigated the recent problem raised in Rubin and Loeb (2014, JCAP, 01, 051) about the kinetic Sunyaev-Zel'dovich effect from the diffuse hot gas in the Local Group, which is predicted to generate a hot spot of a few degrees in size in the cosmic microwave background maps in the direction of M 31, where the free electron optical depth is highest. We also considered whether the same effect in the opposite direction with respect to the M 31 galaxy induces a minimum in temperature in the Planck maps of the sky. We find that the Planck data at 100 GHz show an even stronger effect than that expected.
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页数:4
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