by Ann » Fri Jun 21, 2024 5:48 am
Today's APOD is a nice image, and I'm very glad indeed that Hubble is back in action!
NGC 1546 reminds me somewhat of M63 because of its inclination and its small scattered clusters and thick dust lanes:
But wait, there is something wrong with the comparison of NGC 1546 to M63. Why does the dust of NGC 1546 look so turbulent? It looks like dozens or more of smoking chimneys
are rising from the disk. Even though there are a few smoking chimneys in M63 too, on the whole M63 looks nothing like that. What's going on with NGC 1546?
Could there be more of NGC 1546 than meets the eye in the Hubble picture? Indeed there is!
As you can see, NGC 1546 has a huge massive halo that dwarfs the inner disk within. So, rather than NGC 1546 reminding me of spiral galaxy M63, it reminds me (at least slightly) of the inner gas disk of giant elliptical galaxy M87 (the galaxy with the tremendous central black hole, you know?).
I'm also slightly reminded of the violent starburst in the very central part of spiral galaxy NGC 1808:
However, both the inner gas disk of M87 and the central starburst region of NGC 1808 are very small compared with the overall sizes of these two galaxies. The turbulent disk of gas and dust in NGC 1546 is relatively large compared with the galaxy as a whole.
Still, my explanation for the turbulent nature of the disk of NGC 1546 is that it is caused by the galaxy's central black hole acting up,
or (more likely) the chimneys are remnants of many violent supernovas that followed after a giant burst of star formation in this galaxy's disk.
But wait! There is a third possibility. Maybe NGC 1546 is a ram pressure stripping galaxy? Maybe it is falling through intergalactic space and losing gas as it is falling? Like NGC 4402, which is falling through the intergalactic medium of the Virgo Cluster?
So, hypotheses, hypotheses. Let me end with a look at that lovely little perfectly edge-on background galaxy:
Let's see, where have I seen such a lovely little edge-on background galaxy cosying up to a foreground galaxy before? Oh yes! In the Hubble image of M96:
Gorgeous, isn't it?
Ann
Today's APOD is a nice image, and I'm very glad indeed that Hubble is back in action!
[img3="Hubble's NGC 1546.
Image Credit: NASA, ESA, STScI, David Thilker (JHU)"]https://apod.nasa.gov/apod/image/2406/NGC1546compassHST1024.jpg[/img3]
NGC 1546 reminds me somewhat of M63 because of its inclination and its small scattered clusters and thick dust lanes:
[float=right][img3="Inner disk of M63. Credit: ESA/Hubble & NASA"]https://science.nasa.gov/wp-content/uploads/2023/04/potw1536a-jpg.webp?w=1536&format=webp[/img3][/float][img3="M63. Credit: KPNO/NOIRLab/NSF/AURA/Bruce Hugo and Leslie Gaul/Adam Block"]https://noirlab.edu/public/media/archives/images/wallpaper3/noao-m63hugo.jpg[/img3]
[clear][/clear]
But wait, there is something wrong with the comparison of NGC 1546 to M63. Why does the dust of NGC 1546 look so turbulent? It looks like dozens or more of smoking chimneys β¨οΈ π π are rising from the disk. Even though there are a few smoking chimneys in M63 too, on the whole M63 looks nothing like that. What's going on with NGC 1546?
[img2]https://as1.ftcdn.net/v2/jpg/03/40/27/24/1000_F_340272418_EiXWQtfAD0xbfQInjmBufl1ZbrmRAR9F.jpg[/img2]
Could there be more of NGC 1546 than meets the eye in the Hubble picture? Indeed there is!
[img3="NGC 1546 wide field. Credit: Legacy Surveys / D.Lang (Perimeter Institute) & Meli thev"]https://upload.wikimedia.org/wikipedia/commons/thumb/9/98/NGC_1546_legacy_dr10.jpg/1024px-NGC_1546_legacy_dr10.jpg[/img3]
As you can see, NGC 1546 has a huge massive halo that dwarfs the inner disk within. So, rather than NGC 1546 reminding me of spiral galaxy M63, it reminds me (at least slightly) of the inner gas disk of giant elliptical galaxy M87 (the galaxy with the tremendous central black hole, you know?).
[img3="Inner gas disk of M87. Credit:
Holland Ford, Space Telescope Science Institute/Johns Hopkins University; Richard Harms, Applied Research Corp.; Zlatan Tsvetanov, Arthur Davidsen, and Gerard Kriss at Johns Hopkins; Ralph Bohlin and GeorgeHartig at Space Telescope Science Institute; Linda Dressel and Ajay K.Kochhar at Applied Research Corp. in Landover, Md.; and Bruce Margon fromthe University of Washington in Seattle NASA/ESA"]https://cdn.esahubble.org/archives/images/thumb700x/opo9423b.jpg[/img3]
I'm also slightly reminded of the violent starburst in the very central part of spiral galaxy NGC 1808:
[img3="The central starburst of spiral galaxy NGC 1808. Credit: Jim Flood, an amateur astronomer affiliated with Sperry Observatory at Union College in New Jersey, and Max Mutchler, a member of the Space Telescope Science Institute staff who volunteered to work with Jim"]https://cdn.esahubble.org/archives/images/thumb700x/opo9812b.jpg[/img3]
However, both the inner gas disk of M87 and the central starburst region of NGC 1808 are very small compared with the overall sizes of these two galaxies. The turbulent disk of gas and dust in NGC 1546 is relatively large compared with the galaxy as a whole.
Still, my explanation for the turbulent nature of the disk of NGC 1546 is that it is caused by the galaxy's central black hole acting up,[img2]https://aaah0mnbncqtinas.public.blob.vercel-storage.com/wbNjmOlVX6-no-background-IgSRDClPIX82yxt7iKKLGsyjpaZSQn.png[/img2]
or (more likely) the chimneys are remnants of many violent supernovas that followed after a giant burst of star formation in this galaxy's disk. ππ₯ ππ₯ ππ₯ ππ₯
But wait! There is a third possibility. Maybe NGC 1546 is a ram pressure stripping galaxy? Maybe it is falling through intergalactic space and losing gas as it is falling? Like NGC 4402, which is falling through the intergalactic medium of the Virgo Cluster?
[img3="Ram pressure galaxy NGC 4402. Credit: NASA/ESA/Hubble"]https://www.esa.int/var/esa/storage/images/esa_multimedia/images/2009/09/ngc_4402/9527903-4-eng-GB/NGC_4402_article.jpg[/img3]
So, hypotheses, hypotheses. Let me end with a look at that lovely little perfectly edge-on background galaxy:
[attachment=0]APOD 21 June 2024 detail.png[/attachment]
Let's see, where have I seen such a lovely little edge-on background galaxy cosying up to a foreground galaxy before? Oh yes! In the Hubble image of M96:
[img3="M96 with a lovely little edge-on background galaxy at upper left. Credit: ESO/Oleg Maliy"]https://upload.wikimedia.org/wikipedia/commons/thumb/8/80/NGC_3368_ESO.jpg/800px-NGC_3368_ESO.jpg[/img3]
Gorgeous, isn't it? :D
Ann