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Quasars and Cosmology |
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| Jan10-09, 07:49 PM | #103 |
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Quasars and Cosmology==================================================================== Other references state that NGC4319 is 80 million ly from earth while Mrk 205 is roughly 1 billion ly away. Higher resolution images apparently show no bridge, which could be an optical effects. Apparently there is another galaxy, nearby that may have interacted with NGC4319. NGC 4319 and MK 205 - Galaxies in Draco An Example of the possible Quasar Red Shift Controversy. http://www.kopernik.org/images/archive/n4319.htm |
| Jan10-09, 07:52 PM | #104 |
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Actually, they are. reprocessed images of the HST photo show a clear bridge.
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| Jan10-09, 07:56 PM | #105 |
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Please ensure that this thread stays on topic. Further discussion of Arp's theories here will result in a prompt locking.
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| Jan10-09, 08:00 PM | #106 |
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Edit: Sorry, the above was not posted when I clicked "reply". I will refrain from further discussion of this. |
| Jan10-09, 08:02 PM | #107 |
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(bold added)
Re NGC 4319 and Markarian 205: turbo-1, is there enough data, in the source (FITS) files, of the images presented or referenced in this thread so far for you to be able to do an analysis, to show consistency between them (and where they seem to be inconsistent)? As I count, there are two reproduced in the 1987 Arp & Sulentic ApJ paper, two in the 1987 Sulentic IAU document, several from the HST (and an unknown number from the unknown source). Are there any other readers who have expertise in (digital, astronomical) image analysis? |
| Jan10-09, 08:04 PM | #108 |
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| Jan10-09, 08:06 PM | #109 |
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Please cite some peer-reviewed papers that describe how this "beam" effect arises, and its relation to the aperture/focal ratio of the instrument. You have cited this several times and it is brand-new to me. Of course, my interest in optics only goes back a few decades, and there may be some brand-new modifications of which I am unaware. I am willing to be educated.
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| Jan10-09, 08:16 PM | #110 |
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First, I'd like to apologize. The terminology "beam" is actually not used in optical astronomy. I work in CMB physics, so I tend to use radio/microwave terminology. In optical astronomy, the effect is called the Point Spread Function, often simply abbreviated as "PSF". You can read more up on the theory there. Edit: Usually the PSF of an optical telescope is determined by observing stars. Often it tends to vary slightly within the field, and also, for larger telescopes, will vary just depending upon the inclination of the telescope (the weight of the primary reflector causes it to distort under its own weight). The atmosphere will also cause some degree of aberration that varies with time (hence the utility of adaptive optics). So, most of the time, it's a really bad idea to make any science determinations when you're right at the limit of your PSF/beam: not only is the limit of the beam not very well determined, but it might actually vary either in time or just due to where you're looking. |
| Jan10-09, 08:22 PM | #111 |
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| Jan10-09, 08:23 PM | #112 |
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| Jan10-09, 08:26 PM | #113 |
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| Jan10-09, 08:27 PM | #114 |
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| Jan10-09, 08:27 PM | #115 |
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