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Titlebook: Galactic Bulges; Proceedings of the 1 Herwig Dejonghe,Harm J. Habing Conference proceedings 1993 Kluwer Academic Publishers 1993 Bulge.Gala

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發(fā)表于 2025-3-21 19:40:25 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Galactic Bulges
副標(biāo)題Proceedings of the 1
編輯Herwig Dejonghe,Harm J. Habing
視頻videohttp://file.papertrans.cn/381/380329/380329.mp4
叢書名稱International Astronomical Union Symposia
圖書封面Titlebook: Galactic Bulges; Proceedings of the 1 Herwig Dejonghe,Harm J. Habing Conference proceedings 1993 Kluwer Academic Publishers 1993 Bulge.Gala
描述In the early summer of ‘89 a very informal meeting on the bulge of our Galaxy was held in Leiden. During that meeting Michael Rich proposed 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 location of the meeting was that Ghent is a very beautiful city and had never before hosted an IAU symposium. It could be that this, plus the fact that he is a very keen amateur astronomer led H. M. the King of Belgium to offer his patronage to the meeting - an offer that we gratefully and - we hope - gracefully accepted. The meeting took place at a resort some 15 km outside Ghent. Most participants were housed on the premises - a very convenient situation. This feeling of togeth- erness made up for the small shortcomings of the lecture room, which is normally used as a sports hall. The weather was fair, except on the day of the barbecue when pouring rain forced us to go inside.
出版日期Conference proceedings 1993
關(guān)鍵詞Bulge; Galaxy; Variation; galaxies; milky way
版次1
doihttps://doi.org/10.1007/978-94-011-0922-2
isbn_softcover978-0-7923-2425-6
isbn_ebook978-94-011-0922-2Series ISSN 1743-9213 Series E-ISSN 2352-2186
issn_series 1743-9213
copyrightKluwer Academic Publishers 1993
The information of publication is updating

書目名稱Galactic Bulges影響因子(影響力)




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沙發(fā)
發(fā)表于 2025-3-21 21:36:17 | 只看該作者
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.
板凳
發(fā)表于 2025-3-22 02:10:45 | 只看該作者
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
地板
發(fā)表于 2025-3-22 07:02:45 | 只看該作者
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.
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發(fā)表于 2025-3-22 23:34:56 | 只看該作者
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.
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發(fā)表于 2025-3-23 03:14:46 | 只看該作者
10#
發(fā)表于 2025-3-23 07:28:25 | 只看該作者
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.
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