Arp’s Peculiar Galaxies
Page 10 of 18
Arp observations 91-100 of 171 total to date.
| Thumbnail | Title/link | Arp Category | Date Observed | Observer Description |
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Arp 176 / NGC 4933 | Galaxies with narrow counter-tails | 2024-04-16 23:55:00 | This is a tiny cluster of 3 galaxies: NGC 4933 A/B/C. B is the tail galaxy which appears to be a small elliptical galaxy.. A is the middle, larger, spiral galaxy. C is the dim triangular nub ENE of A. The two brighter galaxies are Magnitude 13, and clearly interacting. C is magnitude 18.5 and does not seem to be interacting with the others. Arp remarks that "Companion galaxy very condensed." Assuming A is an elliptical galaxy, I interpret the remark as applying to the narrowness of the plume as it extends past the A's core, which accounts for the "narrow counter-tail". |
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Arp 178 / NGC 5614, 5615, and 5613 | Galaxies with narrow counter-tails | 2025-07-18 22:44:00 | This is a truly enigmatic Arp object. At first glance it appears to be two galaxies interacting: NGC 5614 (the large galaxy) and NGC 5613 (the medium sized galaxy above it). Unfortunately, the giant plume (which is the predominant "peculiar" feature" doesn't make any sense in that context. It starts to make sense when you realize that the spot on the rim of 5614, close to the right hand edge at the base of the plume, is a dwarf spiral in its own right, NGC 5615. Then, especially after some enhancement, my image reveals some structure: a brighter tidal tail the width of NGC 5615 within the larger, much more diffuse plume that appears nearly structureless. In the first instance, it seems like this was formed by detritus left behind when 5615 was ripped out of a likely orbit (R to L). |
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Arp 181 / NGC 3215-3212 | Galaxies with narrow filaments | 2024-12-25 21:08:00 | We focused on illustrating the key feature that Arp called out: the "narrow filaments" or tidal tails emanating from NGC 3212. He remarked on the "long faint filament extend[ing] westward from south arm". This tests the limits of EAA techniques. While the galaxies themselves are reasonably bright at mag. 10.3 for NGC 3215, and 11.2 for 3212, the surface brightness of the long filament is MUCH dimmer. Note it's barely visible in Arp's plate, and this is one of the few faint details I was not able make readily visible in an inverted version. This despite 56m integration using a mono camera, which is normally more than adequate. While barely visible in the "as captured" EAA positive-image, visibility was enhanced using stretching and sharpening. The "annotated" image came from a 2013 paper in the Monthly Notices of the RAA. This notice, based principally on radio observations, concludes that the interaction has shifted an estimated 90% of the H1 mass outside the optical discs of the two galaxies. The interaction has triggered a burst of star formation activity in two "Tidal Dwarf Galaxies" which peak close to the end of the long filament which Arp called out, labelled TDG and SDSS, respectively. TDG is close to the end of the optical filament but not visible in optical wavelengths; SDSS corresponds to the middle smudge cut off by the western (bottom) border of the comparison images. It is fully visible in the "featured image" reproduced next to the table on wide screen devices. |
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Arp 182 / NGC 7674 and 7675 / Hickson 96 | Galaxies with narrow filaments | 2024-11-03 23:08:00 | Arp 182 displays two faint filaments extending from what otherwise appears to be an intact spiral galaxy (NGC 7674) with a very close companion, and a second spiral much further away (NGC 7675) but likely gravitationally bound to it. Arp calls out the first filament in his remarks: "Long straight, very faint filament like bow wave from comp[anion]." If you imagine that the companion galaxy is a motorboat headed NW (up, left) to pass 7674 on its starboard bow, the "bow wave" leaves a triangular wake behind it. This is an extremely subtle, progressively widening, triangular filament. I believe it's more clear when I render Arp's plate as a positive [image 2 in gallery]. You see both Arp renderings in comparison to my positive image, which, frankly, does not show it. However, gallery image 3 is a negative (invert) of my capture, which does, particularly the southern side of the wake which appears to connect to NGC 7475 (and likely evidence of gravitational interaction). . Much more obvious in my inverted rendering is a semi-circular filament extending NE from 7674 (to the left and up), likely an extension of its bottom, spiral arm. |
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Arp 184 / NGC 1961 | Galaxies with narrow filaments | 2024-02-29 00:00:59 | This was an enjoyable, early capture, and after 40m of integration I shut things down thinking I'd done a great job. However, I hadn't focused on the peculiarity of this galaxy, which was, "Galaxies with narrow filaments". Turns out I had been fooled by the bright galactic center and disk, not recognizing that the filaments were MUCH less bright. My initial attempt with the color image was pretty poor. After using a mono camera starting in late October of 2024, I gained experience in post-processing mono images to bring out faint filaments. So on Election Day (November 5) I decided to convert this image to mono and try the same techniques. They turned out pretty well: the filaments are clearly visible. Luckily, these are the filaments that Arp calls out in the remarks: "Two long straight arms or filaments tangent to NE side of galaxy." Whew! |
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Arp 185 / NGC 6217 | Galaxies with narrow filaments | 2024-05-23 23:56:00 | NGC 6217 is a relatively large and bright barred spiral Arp galaxy, located high in the sky in Ursa Minor. Arp categorizes it as a galaxy with "narrow filaments" and notes in his remarks, "Condensed nucleus. Faint outer arms less curved than inner arms." You know that when the guy with the 200" telescope describes something as "faint", you're in trouble, especially when you're observing on a nearly full-moon night. At the time, I didn't know how to find Arp's remarks so this might have scared me away. However, I was aware of the category, and thought I could see the filaments at capture time. However, in the cold light of day, they're much less evident in the color image than I thought (a common phenomenon in EAA). You can play confirmation-bias with the featured color image and the Arp v color image (2nd in gallery). Fortunately, I've learned that converting a color image to grayscale and inverting it, often helps in this circumstance (first image in gallery). The base of the filament is obvious at the NNW corner of 621 as it exits just above the three bright objects, then takes a wide arc up and to the left (ESE) toward the double-star near the top of the image. The further you go, there's not enough data to resolve it as a "filament", but there's more frequent noise, well above average. Please ignore the faint satellite trail in virtually the same direction. The symmetrical filament out of the SE end of 6217 is much less distinct but still presents a higher noise level. |
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Arp 188 / Tadpole Galaxy / UGC 10214 | Galaxies with narrow filaments | 2024-10-24 20:19:00 | Something dragged out the tail, but it's not immediately apparent what. Arp remarks: "Disturbance inside W arm, filament may originate there." This is a disturbed, barred spiral galaxy. While filament does indeed seem to originate in the western arm, and continue out on the same plane as the disk, stretching out an enormously long "narrow filament". Something else seems to have glommed onto the top of the disk defining a second plane, obscuring a section of the western arm. An incomplete merger? Could the merger be the disturbance that triggered expelling the filament? |
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Arp 189 / Umbrella Galaxy / NGC 4651 | Galaxies with narrow filaments | 2024-05-01 22:38:00 | This is a very bright and reasonably large galaxy, where the "handle", a faint, vertical dust lane, became evident after about 30m of integration. Clouds shut down observing after 55m. Affinity Photo processing of the .png image saved "as adjusted" in Sharpcap makes it more apparent at the cost of a much noisier background. As part of my pre-submission review, I processed the monochrome, inverted version which makes the "handle" even more evident. In most other respects this spiral galaxy appears normal. It is slightly elongated vertically, and the outer arm of the spiral is slightly detached from the rest of the disc, both consistent with a gravitational attraction from the top of the image. There do seem to be some tiny galaxies in the region where the handle terminates, evident in both the color and inverted images. However, I wouldn't want to speculate whether they are attracting the "narrow filament" or some other process is responsible. |
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Arp 199 / NGC 5544-5 | Galaxies with material ejected from nuclei | 2025-09-21 21:07:00 | These two galaxies were discovered by William Herschel on a very productive night in 1785. He originally classified it as a single galaxy. 40 years later his son, John, saw them clearly enough to separate them into two. Arp found the interaction interesting, but seemed to focus on "material ejected from nuclei". |
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Arp 200 / NGC 1134 | Galaxies with material ejected from nuclei | 2026-03-02 20:29:00 | Combining Arp's category (galaxies with "material ejected from nuclei") with his observing remarks: "Splash appearance on W side of galaxy points to low S[urface].B[rightness]. comp[anion galaxy]. 7' S." There's a comparison image in the gallery with arrows pointing out the companion, and a Hubble image follows that removes any doubt that that companion exists. The "splash appearance" is the mottled structure (barely visible in my image) just left of the companion, and behind the companion in the Hubble image. This is classic Arp, who was heavily influenced by Armenian astronomer Viktor Ambartsumian who argued for similar ejections from what we would today call AGN (active galactic nuclei, or supermassive black holes). |