Hubble Space Telescope Imaging of the Central 1 Kiloparsec of M81

Details Hubble Space Telescope Imaging of the Central 1 Kiloparsec of M81 Hubble Space Telescope Imaging of the Central 1 Kiloparsec of M81

Jun 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997apj...481l..71d&link_type=abstract

Astrophysical Journal Letters v.481, p.L71

Astronomy and Astrophysics

Astronomy

36

Galaxies: Individual Messier Number: M81, Galaxies: Individual Ngc Number: Ngc 3031, Galaxies: Nuclei, Galaxies: Seyfert, Galaxies: Spiral, Galaxies: Photometry, Ultraviolet: Galaxies

Scientific paper

M81 is the closest example of a galaxy that exhibits both LINER and Seyfert 1 characteristics. New, post-repair (cycle 5), Hubble Space Telescope imaging observations of the central kpc of M81 are presented, specifically, WFPC2 H alpha and continuum images, a WFPC2 UV continuum (1500 A) image, and a V-band faint object camera (FOC) image. The continuum image shows a number of sinuous dust lanes that wind into the nucleus of M81. The H alpha image reveals a small, ~7" (120 pc), bright, elliptical region of emission that appears to be a nuclear disk. The center of the disklike structure is offset by less than 0."6 (10 pc) from the bright unresolved nucleus. The WFPC2 UV image shows that the disk is not ionized by massive stars. The highest angular resolution observations, obtained with the FOC, allow an upper limit of 0."04 (0.7 pc) to be placed on the size of the nucleus in the V band. The FOC image also shows that there are no stars, star clusters, or additional nuclei visible within the central 4" x 4" region of M81 that are brighter than the galaxy background light.

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