Astronomy and Astrophysics – Astronomy
Scientific paper
May 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aas...180.5403f&link_type=abstract
American Astronomical Society, 180th AAS Meeting, #54.03; Bulletin of the American Astronomical Society, Vol. 24, p.818
Astronomy and Astrophysics
Astronomy
5
Scientific paper
We present HST narrow band PC images of M31 and M51. The center of M31 is completely resolved by the F658N and F547M images. Both images show a bar-like structure with a length of ~ 0.5'' (1.6 parsecs) and a bright resolved ``nucleus'' which is offset from the isophotal (and dynamical) center of the galaxy by ~ 0.2'' (0.65 parsecs). The difference between the [N II] lambda 6584 on-band image and the F547M off-band image shows extended emission across the center of the bar-like structure. We discuss two possible explanations for the morphology of the central region: i) the bright displaced nucleus is the center of a satellite galaxy which has been captured by dynamical friction, and ii) the apparent off-set nucleus is the end of a bar-like structure which is partially obscured by dust associated with the observed emission. Images of M51 were taken through the F502N, F547M, and F664N filters. The continuum image shows a striking X-like absorption feature, most likely due to dust, centered on the nucleus. The most prominent ``dust lane'' divides the nucleus and is perpendicular to thearcsecond, nonthermal radio emission observed with the VLA. The on-band images show strong [O III] and Hα emission perpendicular to the dust lane and aligned with the radio jet. The images do not show a stellar source at the center of the galaxy. The nucleus and central radio source appear to be hidden behind the dust lane which could be an edge-on disk. We briefly discuss future FOS observations of M31 and M51. This work is supported by NASA-GSFC grant NAG 5-1630.
Caganoff Saul
Evans Ian N.
Ford Holland C.
Kriss Gerard Anthony
Tsvetanov Zlatan
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