The Extended Baryonic Halo of NGC 3923
Galaxy halos and their globular cluster systems build up over time by the accretion of small satellites. We can learn about this process in detail by observing systems with ongoing accretion events and comparing the data with simulations. Elliptical shell galaxies are systems that are thought to be...
Main Authors: | Bryan W. Miller, Tomás Ahumada, Thomas H. Puzia, Graeme N. Candlish, Stacy S. McGaugh, J. Christopher Mihos, Robyn E. Sanderson, Mischa Schirmer, Rory Smith, Matthew A. Taylor |
---|---|
Format: | Article |
Language: | English |
Published: |
MDPI AG
2017-07-01
|
Series: | Galaxies |
Subjects: | |
Online Access: | https://www.mdpi.com/2075-4434/5/3/29 |
Similar Items
-
The Baryonic Halos of Isolated Elliptical Galaxies
by: Ricardo Salinas, et al.
Published: (2017-08-01) -
An Excess of Low-mass X-Ray Binaries in the Outer Halo of NGC 4472
by: van Haaften, Lennart M., et al.
Published: (2018) -
The Newtonian and MOND dynamical models of NGC 5128: Investigation of the dark matter contribution
by: Samurović S.
Published: (2016-01-01) -
Revisiting the Globular Cluster Systems of NGC 3258 and NGC 3268
by: Juan Pablo Caso, et al.
Published: (2017-08-01) -
One Piece at a Time—Adding to the Puzzle of S0 Formation
by: Carlos Escudero, et al.
Published: (2017-08-01)