ロード中...
Photometry of Fourteen Main Belt Asteroids
The results of CCD photometry of 14 main belt asteroids obtained between1996 and 2000 are presented. For most of them, the V or R composite lightcurvesand the values of the synodic rotational period are derived. There exists no previousdetermination of the period for 11 of the observed objects.
保存先:
| 出版年: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| 第一著者: | |
| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
Universidad Nacional Autónoma de México
2003
|
| 主題: | |
| オンライン･アクセス: | https://www.redalyc.org/articulo.oa?id=57139106 |
| タグ: |
タグ追加
タグなし, このレコードへの初めてのタグを付けませんか!
|