File:Bengt Strömgren NYWTS.jpg

出自Wikimedia Commons
跳至導覽 跳至搜尋

原始檔案(2,909 × 3,751 像素,檔案大小:1.15 MB,MIME 類型:image/jpeg

說明

說明

添加單行說明來描述出檔案所代表的內容

摘要[編輯]

描述 Bengt Strömgren, astronomer, Yerkes Observatory, Wisconsin / World Telegram & Sun photo by Roger Higgins.
日期
來源 Library of Congress Prints and Photographs Division. New York World-Telegram and the Sun Newspaper Photograph Collection. http://hdl.loc.gov/loc.pnp/cph.3f05797
作者 New York World-Telegram and the Sun staff photographer: Higgins, Roger, photographer.
授權許可
(重用此檔案)
PD [1]
本圖像可以從美國國會圖書館的圖片與照片組獲得,其編號為cph.3f05797
此標籤不表示文件的著作權狀態。任何文件在附有此標籤的同時還需要一個有效的著作權標籤請參閱許可協議說明頁面以了解更多資訊。

العربية  беларуская (тарашкевіца)  বাংলা  čeština  Deutsch  English  español  فارسی  suomi  français  galego  עברית  magyar  Bahasa Indonesia  italiano  日本語  lietuvių  македонски  മലയാളം  Nederlands  polski  português  português do Brasil  română  русский  sicilianu  slovenčina  slovenščina  Türkçe  українська  简体中文  繁體中文  +/−

Deutsch: Bengt Georg Daniel Strömgren (* 21. Januar 1908 in Göteborg, Schweden;
English: Bengt Georg Daniel Strömgren ( January 21 1908July 4 1987) was a Danish astronomer and astrophysicist.
Français : Bengt Georg Daniel Strömgren ( 2 janvier 1908-4 juillet 1987) est un astronome et astrophysicien danois.
Italiano: Nacque a Göteburg, da Hedvig ed Elis Strömgren, professore di astronomia presso l'Università di Copenhagen, e direttore dell'osservatorio universitario di Copenhagen. Bengt crebbe circondato da scienziati, dai loro assistenti, e vari ospiti. Suo padre spinse Bengt verso una vita dedicata alla scienza, ed il primo articolo del giovane Strömgren fu pubblicato quando aveva appena 14 anni. Fu promosso al liceo nel 1925, ed entrò all'Università di Copenhagen. Due anni più tardi, si laureò in astronomia e in fisica atomica, e negli anni seguenti, portò a termine un dottorato, che ottenne il massimo dei voti nel Dicembre 1929, quando aveva 21 anni.
日本語: ベンクト・ストレームグレン(Bengt Georg Daniel Strömgren , 1908年1月21日- 1987年7月4日) はデンマーク天体物理学者である。散光星雲(輝線星雲)の発光原因が誕生まもない恒星が発する紫外線によって電離されたHII領域(ストレームグレン球)であることを示した。

(This summary was created using Commons SumItUp) de:Bengt Strömgren en:Bengt_Strömgren fr:Bengt Strömgren it:Bengt Georg Daniel Strömgren ja:ベンクト・ストレームグレン

授權條款[編輯]

Public domain This work is from the New York World-Telegram and Sun collection at the Library of Congress. According to the library, there are no known copyright restrictions on the use of this work.
This photograph is a work for hire created prior to 1968 by a staff photographer at New York World-Telegram & Sun. It is part of a collection donated to the Library of Congress and per the instrument of gift it is in the public domain.

Photographs in this collection other than those identified by such stamps as "World-Telegram photo" or "World-Telegram photo by Ed Palumbo" might not be in the public domain. Works within the collection may be attributed to other news services that retain copyright, works of the U.S. government that are in the public domain in the US, or works with no attribution for which copyright cannot be determined.

檔案歷史

點選日期/時間以檢視該時間的檔案版本。

日期/時間縮⁠圖尺寸用戶備⁠註
目前2007年1月16日 (二) 15:14於 2007年1月16日 (二) 15:14 版本的縮圖2,909 × 3,751(1.15 MB)Davepape對話 | 貢獻==Summary== {{Information |Source=Library of Congress Prints and Photographs Division. New York World-Telegram and the Sun Newspaper Photograph Collection. http://hdl.loc.gov/loc.pnp/cph.3f05797 |Description= Bengt Strömgren, a

下列頁面有用到此檔案:

全域檔案使用狀況

以下其他 wiki 使用了這個檔案:

詮釋資料