Timeline for How do we know Milky Way is a 'barred' spiral galaxy?
Current License: CC BY-SA 4.0
11 events
| when toggle format | what | by | license | comment | |
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| Sep 28, 2021 at 13:12 | history | edited | Walter | CC BY-SA 4.0 |
deleted 6 characters in body
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| Sep 28, 2021 at 6:29 | history | edited | Walter | CC BY-SA 4.0 |
added RC luminosity evidence
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| Apr 16, 2019 at 11:06 | history | edited | Peter Erwin | CC BY-SA 4.0 |
Spelling correction.
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| Jun 10, 2015 at 12:04 | comment | added | Walter | @RobJeffries psst about that walter here. | |
| Jun 10, 2015 at 10:06 | comment | added | ProfRob | Ah that "Walter"! I'll check it out - I am interested in young moving groups and similar kinematic structures. | |
| Jun 10, 2015 at 9:50 | comment | added | Walter | @RobJeffries Look at my article and any quoting it. | |
| Jun 9, 2015 at 6:05 | comment | added | ProfRob | Can you provide something that backs up the item about velocity clumps in the solar neighbourhood are due to resonance with the bar - genuinely interested. | |
| Sep 13, 2014 at 22:52 | comment | added | Wayfaring Stranger | Bar at Milky Way's heart revealed (August 2005): newscientist.com/article/… | |
| Dec 30, 2013 at 4:43 | vote | accept | Cheeku | ||
| Dec 29, 2013 at 19:01 | comment | added | Alexey Bobrick | Nice answer! Can you add a few references to articles or instruments concerning at least some of these things you mention: gas velocity measurements, solar neighbourhood assymetries and clumping, bar parameters fitting. | |
| Dec 29, 2013 at 16:25 | history | answered | Walter | CC BY-SA 3.0 |