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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書目名稱Galactic Bulges影響因子(影響力)




書目名稱Galactic Bulges影響因子(影響力)學(xué)科排名




書目名稱Galactic Bulges網(wǎng)絡(luò)公開度




書目名稱Galactic Bulges網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Galactic Bulges被引頻次




書目名稱Galactic Bulges被引頻次學(xué)科排名




書目名稱Galactic Bulges年度引用




書目名稱Galactic Bulges年度引用學(xué)科排名




書目名稱Galactic Bulges讀者反饋




書目名稱Galactic Bulges讀者反饋學(xué)科排名

Custodian

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.

驚奇

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

保守黨

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

Folklore

Folklore

殘忍

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

ALT

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.