This page describes an image Stellar birth environment
Image caption:
Snapshot of the formation of multiple protostars in the Orion Molecular Clouds with a closer look at each of them with the Atacama Large Millimeter/submillimeter Array and Very Large Array. Such an image provides unique insights of the process and early stages of star formation as well as the influence of the parent cloud in which they form.
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Image credit:
ALMA (ESO/NAOJ/NRAO), J. Tobin; NRAO/AUI/NSF, S. Dagnello; Herschel/ESA Credit Link
Related glossary terms:
Protostar
, Star Formation
Categories:
Milky Way and Interstellar Medium
, Stars
Image license: Creative Commons Attribution 3.0 Unported Creative Commons Attribution 3.0 Unported icons
The media file captions presented on the OAE website were written, translated and reviewed by a collective effort from the OAE, the OAE Centers and Nodes, the OAE National Astronomy Education Coordinators (NAECs) and other volunteers. You can find a full list of credits for our translation project here. All media file captions are released under a Creative Commons CC BY-4.0 license and should be credited to "IAU OAE". The media files themselves may have different licenses (see above) and should be credited as listed above under "credit".
If you notice a factual error in this caption or an error in any of its translations then please get in touch.
Captions in Different Languages:
Image caption: Istantanea della formazione di più protostelle nelle nubi molecolari di Orione, con uno sguardo ravvicinato a ciascuna di esse con l'Atacama Large Millimeter/submillimeter Array e il Very Large Array. Questa immagine offre una visione unica del processo e delle prime fasi di formazione delle stelle, nonché dell'effetto della nube madre in cui si formano.
Image credit: ALMA (ESO/NAOJ/NRAO), J. Tobin; NRAO/AUI/NSF, S. Dagnello; Herschel/ESA
Related glossary terms: Formazione delle stelle , Protostella Caption translation status: Approved by a reviewer
Caption translators: Giuliana Giobbi
Caption reviewers: Rosa Valiante, Rodolfo Canestrari
Image caption: 使用阿塔卡马大型毫米/亚毫米波阵（ALMA）和甚大阵（VLA），拍摄了猎户座分子云中多颗原恒星形成的快照，更仔细地观察了每颗原恒星。对于恒星形成的过程和早期阶段，以及恒星从中形成的母云所产生的影响，这样的图像提供了独特的见解。
Image credit: ALMA (ESO/NAOJ/NRAO), J. Tobin; NRAO/AUI/NSF, S. Dagnello; Herschel/ESA
Related glossary terms: 原恒星 , 恒星形成 Caption translation status: Not yet approved by a reviewer
Caption translators: Bao Lizhuo
Image caption: 使用阿塔卡馬大型毫米/亞毫米波陣（ALMA）和甚大陣（VLA），拍攝了獵戶座分子雲中多顆原恆星形成的快照，更仔細地觀察了每顆原恆星。對於恆星形成的過程和早期階段，以及恆星從中形成的母雲所產生的影響，這樣的圖像提供了獨特的見解。
Image credit: ALMA (ESO/NAOJ/NRAO), J. Tobin; NRAO/AUI/NSF, S. Dagnello; Herschel/ESA
Related glossary terms: 原恆星 , 恆星形成 Caption translation status: Not yet approved by a reviewer
Caption translators: An automated transliteration from the simplified Chinese translation by - Bao Lizhuo
