Файл:The Many Layers of NGC 1808 (iotw2320a).jpg
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ТасвирThe Many Layers of NGC 1808 (iotw2320a).jpg |
English: NGC 1808 is a barred spiral galaxy located in the southern constellation Columba (the dove). This image was captured using the Dark Energy Camera (DECam), which is mounted on the Víctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory (CTIO), a Program of NSF’s NOIRLab, in Chile. The core of NGC 1808 is thought to house a supermassive black hole, characterized by its accretion of material and higher-than-normal brightness. The smoldering center is closely surrounded by a faint blue ring populated with star clusters and supernova remnants. This region is defined by its starburst activity, producing an exceptional number of hot, bright, young stars. The abundance of rapid star formation is thought to be the result of past tidal interactions with the nearby galaxy NGC 1792. Laced throughout this middle region of NGC 1808 are dark dust lanes resulting from large outflows of hydrogen gas from the galactic nucleus. The softly glowing outer arms surrounding the galaxy are slightly warped, again pointing to tidal interactions with NGC 1792. Such an interaction could have created the asymmetrical shape of NGC 1808 and hurled gas towards the nucleus, igniting the rapid star formation in its surrounding ring.You can find a square view of this Image of the Week here.Image processing: R. Colombari and M. Zamani (NSF’s NOIRLab) |
Дата | 17 май 2023 (дата загрузки) |
Чыганак | The Many Layers of NGC 1808 |
Автор | Dark Energy Survey/DOE/FNAL/DECam/CTIO/NOIRLab/NSF/AURA |
Башка юрамалар |
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Лицензияләү
This media was created by the National Optical-Infrared Astronomy Research Laboratory (NOIRLab).
Their website states: "Unless specifically noted, the images, videos, and music distributed on the public NOIRLab website, along with the texts of press releases, announcements, images of the week and captions; are licensed under a Creative Commons Attribution 4.0 International License, and may on a non-exclusive basis be reproduced without fee provided the credit is clear and visible." To the uploader: You must provide a link (URL) to the original file and the authorship information if available. | |
Этот файл доступен по лицензии Creative Commons Attribution 4.0 International
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Кулланылган программа | Adobe Photoshop 24.2 (Windows) |
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Санлаштыру вакыты | 14 мар 2023, 18:43 |
Файл үзгәреше датасы һәм вакыты | 24 мар 2023, 22:49 |
Дата последнего изменения метаданных | 24 мар 2023, 22:49 |
Поставщик, кто предоставил изображение | Dark Energy Survey/DOE/FNAL/DECam/CTIO/NOIRLab/NSF/AURA |
Чыганак | NSF's NOIRLab |
Уникальный идентификатор исходного документа | xmp.did:b65f57ce-f572-324f-9d0f-3ce2b37c5f3b |
Кыска исем |
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Сурәт исеме |
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Иң мөһиме | NGC 1808 |
Элемтә өчен мәгълүмат |
950 North Cherry Ave. Tucson, AZ, 85719 USA |
Куллану шартлары |
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Чын вакыты | 17 май 2023, 06:00 |
Примечание JPEG-файла | NGC 1808 is a barred spiral galaxy located in the southern constellation Columba (the dove). This image was captured using the Dark Energy Camera (DECam), which is mounted on the Víctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory (CTIO), a Program of NSF’s NOIRLab, in Chile. The core of NGC 1808 is thought to house a supermassive black hole, characterized by its accretion of material and higher-than-normal brightness. The smoldering center is closely surrounded by a faint blue ring populated with star clusters and supernova remnants. This region is defined by its starburst activity, producing an exceptional number of hot, bright, young stars. The abundance of rapid star formation is thought to be the result of past tidal interactions with the nearby galaxy NGC 1792. Laced throughout this middle region of NGC 1808 are dark dust lanes resulting from large outflows of hydrogen gas from the galactic nucleus. The softly glowing outer arms surrounding the galaxy are slightly warped, again pointing to tidal interactions with NGC 1792. Such an interaction could have created the asymmetrical shape of NGC 1808 and hurled gas towards the nucleus, igniting the rapid star formation in its surrounding ring. You can find a square view of this Image of the Week here. Image processing: R. Colombari and M. Zamani (NSF’s NOIRLab) |