this post was submitted on 25 Mar 2025
36 points (100.0% liked)
[Migrated, see pinned post] Casual Conversation
3363 readers
1 users here now
We moved to [email protected] please look for https://lemm.ee/post/66060114 in your instance search bar
Share a story, ask a question, or start a conversation about (almost) anything you desire. Maybe you'll make some friends in the process.
RULES
- Be respectful: no harassment, hate speech, bigotry, and/or trolling.
- Encourage conversation in your OP. This means including heavily implicative subject matter when you can and also engaging in your thread when possible.
- Avoid controversial topics (e.g. politics or societal debates).
- Stay calm: Don’t post angry or to vent or complain. We are a place where everyone can forget about their everyday or not so everyday worries for a moment. Venting, complaining, or posting from a place of anger or resentment doesn't fit the atmosphere we try to foster at all. Feel free to post those on [email protected]
- Keep it clean and SFW
- No solicitation such as ads, promotional content, spam, surveys etc.
Casual conversation communities:
Related discussion-focused communities
founded 2 years ago
MODERATORS
you are viewing a single comment's thread
view the rest of the comments
view the rest of the comments
Recent stellar evolution computations show that the blue supergiant (BSG) stars could come from two distinct populations: a first group arising from massive stars that just left the main sequence and are crossing the Hertzsprung–Russell diagram (HRD) towards the red supergiant (RSG) branch, and a second group coming from stars that have lost considerable amount of mass during the RSG stage and are crossing the HRD for a second time towards the blue region.
Wow. This goes well beyond "casual conversation" 😅
But your article is saying that it happens, and a large factor is mass being ejected, and I can understand that I suppose. Cool!
Well...
I started casual...