Hubble Space Telescope Observations of the Double Nucleus of NGC 4486B

Details Hubble Space Telescope Observations of the Double Nucleus of NGC 4486B Hubble Space Telescope Observations of the Double Nucleus of NGC 4486B

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apj...471l..79l&link_type=abstract

Astrophysical Journal Letters v.471, p.L79

Astronomy and Astrophysics

Astronomy

63

Galaxies: Nuclei, Galaxies: Photometry, Galaxies: Structure

Scientific paper

Hubble Space Telescope WFPC2 images show that the low-luminosity elliptical galaxy companion to M87, NGC 4486B, has a double nucleus that resembles the one discovered in M31. The NGC 4486B nucleus comprises two peaks separated by ~0."15 or 12 pc. Neither peak is coincident with the galaxy photocenter, which falls between them. The nuclear morphology is independent of color; thus, the double structure is not likely to arise from dust absorption. It is also unlikely that the peaks are a binary stellar system (such as an ongoing merger of the nucleus of a less luminous system with the nucleus of NGC 4486B), since the decay timescale is short (<108 yr) and the present environment of NGC 4486B should inhibit mergers. We suggest that the nuclear morphology of NGC 4486B may be explained by the eccentric-disk model of Tremaine, which was originally advanced to account for the central structure of M31. This model requires that NGC 4486B contains a central massive dark object, which is suggested by the spectroscopic observations of Kormendy et al. The eccentric disk might be related to the symmetric disk seen at larger radii.

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