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Figure 1:
NGC 2859, a prototypical double-barred galaxy first noted by
Kormendy (1979). The figure shows logarithmic R-band contours,
displaying both the outer bar and the inner bar inside it, along with
ellipse fits to the isophotes (upper right) and an unsharp mask
(lower right) of the inner bar, with hints of spiral arms just outside
it. The dashed circles on the unsharp mask have, from the inside out,
radii =
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Figure 2: Examples of the appearance of "normal'' (i.e., large-scale) bars in unsharp masks. For each galaxy I show logarithmically scaled isophotes (top) and an unsharp mask from the same image (bottom). a) The outer bar of the double-barred SB0 galaxy NGC 4340; traces of a ring surrounding the bar can also be seen (R-band image from the MDM Telescope). b) NGC 4643, an example of an extremely narrow bar in an SB0/a galaxy, with the central "spine'' of the bar showing up clearly in the unsharp mask, along with very faint traces of a thin ring (R-band image from Erwin & Sparke 2003). |
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Figure 3: As for Fig. 2, but now showing inner bars from double-barred galaxies. a) NGC 1543, where the narrow inner bar is strikingly similar to the (large-scale) bar of NGC 4643 in Fig. 2 (WFPC2 F814W image). b) NGC 6684, an inner bar with a more typical unsharp mask appearance (WFPC2 F814W image). c) NGC 4340, where the inner bar is surrounded by an elliptical stellar nuclear ring (R-band image from the MDM Telescope). |
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Figure 4:
Example of a single-barred galaxy where a nuclear
ring masquerades as an inner bar. The SBa galaxy NGC 2273 was listed
as double-barred by Mulchaey et al. (1997) on the basis of ellipse fits (upper
right: black = K-band fits to their image, gray = HST
H-band fits) and the appearance of their K-band image (upper
left). However, an HST NICMOS2 H-band image (lower left)
and its unsharp mask (lower right) show that the "inner bar'' (
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Figure 5:
Another example of a nuclear ring masquerading as an inner
bar. Here, the SB0 galaxy NGC 4371 shows three distinct peaks in
ellipse fits to ground-based images (upper right: black =
ground-based R-band fits, gray = WFPC2 V-band fits; both
from Erwin & Sparke 1999), which led Wozniak et al. (1995) to suggest that it was
triple-barred. The R-band images (upper and lower left) do
indeed show a prominent inner elliptical feature with
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Figure 6:
Another example of how ellipse fits can misleadingly suggest
two bars in a single-barred galaxy: in this case, a false "outer
bar'' signature is produced by spiral arms in the SABc galaxy
NGC 1667. a) Logarithmically spaced K-band isophotes
(from the image of Mulchaey et al. 1997), along with ellipse fits
b) to the same image (black points) plus ellipse fits to the
NICMOS2 H-band image (gray points). Two strong ellipticity peaks
are present, suggesting a possible double-barred galaxy
(e.g., Laine et al. 2002): an "outer bar'' with
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