The dark matter distribution of NGC 5921
We used the neutral atomic hydrogen data of the Very Large Array for the spiral galaxy NGC 5921 with z = 0.0045 at the distance of 22.4 Mpc, to investigate the nature of dark matter. The investigation was based on two theories, namely, dark matter and Modified Newtonian Dynamics (MOND). We presented...
Saved in:
Main Authors: | Ali, Israa Abdulqasim Mohammed, Hashim, Norsiah, Abidin, Zamri Zainal |
---|---|
Format: | Article |
Published: |
Springer Verlag (Germany)
2018
|
Subjects: | |
Online Access: | http://eprints.um.edu.my/22559/ https://doi.org/10.1007/s12648-017-1119-7 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Dark Matter in the Central Region of NGC 3256
by: Ali, Israa Abdulqasim Mohammed, et al.
Published: (2018) -
Dark matter distributions in the central region of late type NGC3256 and NGC4321 Galaxies / Israa Abdulqasim Mohammed Ali
by: Israa Abdulqasim , Mohammed Ali
Published: (2018) -
Dark matter in the Central Region of NGC 3256
by: Israa Abdulqasim Mohammed Ali,, et al.
Published: (2018) -
A comprehensive analysis using 9 dark matter halo models on the spiral galaxy NGC 4321
by: Tan, Wei Shen, et al.
Published: (2022) -
Kennicutt-Schmidt Law in the Central Region of NGC 4321 as Seen by ALMA
by: Azeez, J.H., et al.
Published: (2016)