by Ann » Thu Jun 15, 2023 9:55 am
M15: Dense Globular Star Cluster with Planetary Nebula Pease 1.
Image Credit: NASA, ESA, Hubble Legacy Archive; Processing: Ehsan Ebrahimian
M15 and NGC 46 are the only clusters I know of that contain a planetary nebula. And NGC 2436 isn't even a member of NGC 2436 but a line-of-sight foreground object!
It's strange that planetary nebulas are so rare in rich clusters, isn't it? Because the way I understand it, all hydrogen-fusing stars will eventually turn into white dwarfs. Then surely they should go through a planetary nebula phase, too? Or maybe the smallest stars will not get extremely hot inside, so they won't do a good job of ionizing the fairly small amounts of gas they will expel when they shrug off their outer layers? Still though, that sounds weird. Surely the core of a puny little M-type dwarf is at least as hot as the photosphere of a mighty O-star?
I said that planetary nebula NGC 2436, which appears to belong to M46, is actually only a foreground object. Yes, but there is another planetary nebula that is really inside M46, or rather, this particular object that is inside M46 is a proto-planetary nebula!
Foreground planetary nebula NGC 2436
and true M46 member, protoplanetary nebula, the Calabash. Credit: NOIRLab.
Read about the Calabash Nebula in M46
here, and read about Pease 1 in globular cluster M15
here.
And don't even get me started on mapped color!!!
Ann
[float=left][attachment=1]M15-3_1024[1].jpg[/attachment][c][size=85][color=#0040FF]M15: Dense Globular Star Cluster with Planetary Nebula Pease 1.
Image Credit: NASA, ESA, Hubble Legacy Archive; Processing: Ehsan Ebrahimian[/color][/size][/c][/float][float=right][img3="Rich open cluster M46 with non-member planetary nebula NGC 2436. Image credit: N.A.Sharp/NOIRLab/NSF/AURA"]https://noirlab.edu/public/media/archives/images/thumb700x/noao-m46.jpg[/img3][/float]
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M15 and NGC 46 are the only clusters I know of that contain a planetary nebula. And NGC 2436 isn't even a member of NGC 2436 but a line-of-sight foreground object! :facepalm:
It's strange that planetary nebulas are so rare in rich clusters, isn't it? Because the way I understand it, all hydrogen-fusing stars will eventually turn into white dwarfs. Then surely they should go through a planetary nebula phase, too? Or maybe the smallest stars will not get extremely hot inside, so they won't do a good job of ionizing the fairly small amounts of gas they will expel when they shrug off their outer layers? Still though, that sounds weird. Surely the core of a puny little M-type dwarf is at least as hot as the photosphere of a mighty O-star?
I said that planetary nebula NGC 2436, which appears to belong to M46, is actually only a foreground object. Yes, but there is another planetary nebula that is really inside M46, or rather, this particular object that is inside M46 is a proto-planetary nebula!
[float=left][attachment=0]Planetary and protoplanetary nebula in M46 NOIRLab.png[/attachment][c][size=85][color=#0040FF]Foreground planetary nebula NGC 2436
and true M46 member, protoplanetary nebula, the Calabash. Credit: NOIRLab.[/color][/size][/c][/float]
[clear][/clear]
Read about the Calabash Nebula in M46 [url=https://en.wikipedia.org/wiki/Calabash_Nebula]here[/url], and read about Pease 1 in globular cluster M15 [url=https://en.wikipedia.org/wiki/Pease_1]here[/url].
And don't even get me started on mapped color!!!
Ann