by Ann » Wed Jun 12, 2024 6:18 am
Amazing! When I first saw the pink cloud in M37, I just couldn't understand what it was. It's a planetary nebula! It is very large, it is very old (the oldest known planetary?), it sits in a ~500 million year old cluster, and the progenitor star had a mass of about ∼2.8 M
☉, which would make it a star of late type B (B8 or B9).
The huge planetary nebula in M37 has been a planetary nebula for a long time (a million years???), but its presence in this cluster still tells us something about how long a late type B star with a mass of some 2.8 M
☉ can be expected to live, its red gianthood included.
Ann
[quote=starsurfer post_id=339537 time=1717799056 user_id=137896]
[size=120][b]M37[/b][/size]
[url]https://www.astrobin.com/e90jkf/[/url]
Copyright: Antoine and Dalia Grelin
kkYsOQppC5W6_2560x0_qNFj77Wg.jpg
M37 is one of the few open clusters known to [url=https://arxiv.org/abs/2208.06101]contain a planetary nebula[/url], which is catalogued as IPHASX J055226.2+323724.
[/quote]
Amazing! When I first saw the pink cloud in M37, I just couldn't understand what it was. It's a planetary nebula! It is very large, it is very old (the oldest known planetary?), it sits in a ~500 million year old cluster, and the progenitor star had a mass of about ∼2.8 M[sub]☉[/sub], which would make it a star of late type B (B8 or B9).
The huge planetary nebula in M37 has been a planetary nebula for a long time (a million years???), but its presence in this cluster still tells us something about how long a late type B star with a mass of some 2.8 M[sub]☉[/sub] can be expected to live, its red gianthood included.
Ann