Research output: Contribution to journal › Article › peer-review
Results of photometric (in color bands B, V, and R(c)) and kinematic studies of the peculiar galaxy NGC 2748 are presented. The mass distribution is represented by two-component model consisting of an exponential disk and a spherical halo. It is shown that the main observational features of NGC 2748 - in particular, the presence of diffuse formations extended along the minor axis and the existence of a radial velocity gradient along the minor axis - are most likely a consequence of accretion onto the galaxy of gas from a dwarf satellite.
Original language | Undefined |
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Pages (from-to) | 36-43 |
Number of pages | 8 |
Journal | АСТРОНОМИЧЕСКИЙ ЖУРНАЛ |
Volume | 73 |
Issue number | 1 |
State | Published - 1996 |
ID: 32253755