Astronomy and Astrophysics – Astrophysics
Scientific paper
1996-06-22
Astronomy and Astrophysics
Astrophysics
14 pages, LaTeX, Figure 4 included, Postscript Figs. 1-3 available at ftp://astro.nmsu.edu/pub/JASON/A1795/, accepted for publ
Scientific paper
10.1086/310219
We present WFPC2 images of the core of the cooling flow cD galaxy in Abell 1795. An irregular, asymmetric dust lane extends 7 \h75 kpc in projection to the north-northwest. The dust shares the morphology observed in the H$\alpha$ and excess UV emission. We see both diffuse and knotty blue emission around the dust lane, especially at the ends. The dust and emission features lie on the edge of the radio lobes, suggesting star formation induced by the radio source or the deflection of the radio jets off of pre-existing dust and gas. We measure an apparent R$_V$ significantly less than 3.1, implying that the extinction law is not Galactic in the dust lane, or the presence of line emission which is proportional to the extinction. The dust mass is at least 2$\times10^{5} h_{75}^{-2}$ M\solar\ and is more likely to be 6.5$\times10^{5} h_{75}^{-2}$ M\solar.
Garasi Chris
Holtzman Jon
IDT the WFPC-2
Pinkney Jason
Watson Alan M.
No associations
LandOfFree
WFPC2 Observations of the Cooling Flow Elliptical in Abell 1795 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with WFPC2 Observations of the Cooling Flow Elliptical in Abell 1795, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and WFPC2 Observations of the Cooling Flow Elliptical in Abell 1795 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-76392