Timing argument take on the Milky Way and Andromeda past encounter

被引:6
|
作者
Benisty, David [1 ,2 ,3 ,4 ]
机构
[1] Frankfurt Inst Adv Studies, Ruth Moufang Str 1, D-60438 Frankfurt, Germany
[2] Ben Gurion Univ Negev, Phys Dept, IL-84105 Beer Sheva, Israel
[3] Univ Cambridge, Kavli Inst Cosmol KICC, Madingley Rd, Cambridge CB3 0HA, England
[4] Univ Cambridge, Ctr Math Sci, DAMTP, Wilberforce Rd, Cambridge CB3 0WA, England
关键词
celestial mechanics; cosmology: miscellaneous; Local Group; LOCAL HUBBLE FLOW; DARK ENERGY; DISTANCE; GRAVITY; MODEL;
D O I
10.1051/0004-6361/202142096
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The two-body problem of the M31 and Milky Way (MW) galaxies with a cosmological constant background is studied, with an emphasis on the possibility that they experienced a past encounter (PE). Past encounters are possible only for a nonzero transverse velocity, and their viability is subject to observations of the imprints of such near collisions. By implementing the timing argument (TA) for two isolated point bodies, it is shown that if M31 and the MW had experienced a PE, then the predicted mass of the Local Group (LG) would be twice larger. This predicted mass is too large and implies that the MW and M31 galaxies would have collided at similar to 8 Gys. Therefore, the TA analysis shows that a PE is not possible for the LG system.
引用
收藏
页数:4
相关论文
共 50 条
  • [21] The Milky Way's cannibalistic past
    Anon
    Scientific American, 2001, 284 (06)
  • [22] The Milky Way and Andromeda galaxies in a constrained hydrodynamical simulation: Morphological evolution
    Scannapieco, Cecilia
    Creasey, Peter
    Nuza, Sebastián E.
    Yepes, Gustavo
    Gottlöber, Stefan
    Steinmetz, Matthias
    1600, EDP Sciences (577):
  • [23] Does the dwarf galaxy system of the Milky Way originate from Andromeda?
    Fouquet, Sylvain
    Hammer, Francois
    Yang, Yanbin
    Puech, Mathieu
    Flores, Hector
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2012, 427 (02) : 1769 - 1783
  • [24] Milky Way and Andromeda analogues from the TNG50 simulation
    Pillepich, Annalisa
    Sotillo-Ramos, Diego
    Ramesh, Rahul
    Nelson, Dylan
    Engler, Christoph
    Rodriguez-Gomez, Vicente
    Fournier, Martin
    Donnari, Martina
    Springel, Volker
    Hernquist, Lars
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2024, 535 (02) : 1721 - 1762
  • [25] Andromeda and the Milky Way: Twin sisters, distant relations, or strangers in the night?
    McConnachie, A.
    Richardson, J.
    Mackey, D.
    ASSEMBLING THE PUZZLE OF THE MILKY WAY, 2012, 19
  • [26] The Milky Way and Andromeda galaxies in a constrained hydrodynamical simulation: morphological evolution
    Scannapieco, Cecilia
    Creasey, Peter
    Nuza, Sebastian E.
    Yepes, Gustavo
    Gottloeber, Stefan
    Steinmetz, Matthias
    ASTRONOMY & ASTROPHYSICS, 2015, 577
  • [27] Equilibrium disk-bulge-halo models for the Milky Way and Andromeda galaxies
    Widrow, LM
    Dubinski, J
    ASTROPHYSICAL JOURNAL, 2005, 631 (02): : 838 - 855
  • [28] Modeling mass independent of anisotropy: A comparison between Andromeda and Milky Way satellites
    Wolf, J.
    HIGHLIGHTS OF ASTRONOMY, VOL 15, 2010, 15 : 79 - 79
  • [29] Future merger of the Milky Way with the Andromeda galaxy and the fate of their supermassive black holes
    Schiavi, Riccardo
    Capuzzo-Dolcetta, Roberto
    Arca-Sedda, Manuel
    Spera, Mario
    ASTRONOMY & ASTROPHYSICS, 2020, 642
  • [30] COMPARING M31 AND MILKY WAY SATELLITES: THE EXTENDED STAR FORMATION HISTORIES OF ANDROMEDA II AND ANDROMEDA XVI
    Weisz, Daniel R.
    Skillman, Evan D.
    Hidalgo, Sebastian L.
    Monelli, Matteo
    Dolphin, Andrew E.
    McConnachie, Alan
    Bernard, Edouard J.
    Gallart, Carme
    Aparicio, Antonio
    Boylan-Kolchin, Michael
    Cassisi, Santi
    Cole, Andrew A.
    Ferguson, Henry C.
    Irwin, Mike
    Martin, Nicolas F.
    Mayer, Lucio
    McQuinn, Kristen B. W.
    Navarro, Julio F.
    Stetson, Peter B.
    ASTROPHYSICAL JOURNAL, 2014, 789 (01):