notable
发表于 2025-3-21 19:40:25
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Custodian
发表于 2025-3-21 21:36:17
Dynamics of the Galactic Bulgeng fairly rapidly. To date, there is little evidence for triaxiality in the stellar kinematics: the available stellar velocities are consistent with Kent’s (1992) oblate model. This unsatisfactory situation is expected to improve rapidly.
惊奇
发表于 2025-3-22 02:10:45
1743-9213 to hold a more properly organised symposium on "Galactic Bulges" in a few years time. After some discussion a Scientific Organising Committee was founded and after some manoeuvring a chairman was chosen, a local organiser was assigned and two editors were given instructions. A good thing about the l
保守党
发表于 2025-3-22 07:02:45
Object-Oriented Transaction-Level Modellingike Rich, Don Terndrup, and Jay Frogel. But any errors, and especially any prejudices, are purely my own. And in my reading I have undoubtedly missed some important papers, but I hope that their authors will forgive me.
Commodious
发表于 2025-3-22 09:05:03
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Folklore
发表于 2025-3-22 16:10:48
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Folklore
发表于 2025-3-22 20:17:11
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残忍
发表于 2025-3-22 23:34:56
Olga Barrera,Alan Cocks,Alan Ponterity function in the central 200 pc resembles that recently found in M32 and M31 bulge fields. Depending on how one interprets the extended giant branch, the population may be intermediate age with some ongoing star formation, or mostly old and metal rich, with star formation confined to the nucleus.
高原
发表于 2025-3-23 03:14:46
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ALT
发表于 2025-3-23 07:28:25
The Stellar Population of the Inner 200 Parsecsity function in the central 200 pc resembles that recently found in M32 and M31 bulge fields. Depending on how one interprets the extended giant branch, the population may be intermediate age with some ongoing star formation, or mostly old and metal rich, with star formation confined to the nucleus.