English: NGC3190, a spiral galaxy of type SA(s)a in the constellation Leo, was imaged during engineering work at the KPNO Mayall 4-meter telescope in January of 2001. The large size of the telescope and the smaller format imager used for test work combine to make the field of view only just the size of the galaxy itself. Multiple exposures on this faint galaxy took a total of 3000s in the blue (B) band, 2000s in green (V) and 1000s in red (R). NGC3190 in fact forms a small group (Hickson 44, Arp 316) with NGC3193 to the east, NGC3187 to the west, and NGC3185, significantly further away to the southwest. Interestingly, NGC3189 refers to the south-west (lower right) part of NGC3190. The strong dust lane down the middle apparently misled the catalog compilers into giving it two separate numbers. NGC3190 also contains an active galactic nucleus.
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.
делиться произведением – копировать, распространять и передавать данное произведение
создавать производные – переделывать данное произведение
При соблюдении следующих условий:
атрибуция – Вы должны указать авторство, предоставить ссылку на лицензию и указать, внёс ли автор какие-либо изменения. Это можно сделать любым разумным способом, но не создавая впечатление, что лицензиат поддерживает вас или использование вами данного произведения.
https://creativecommons.org/licenses/by/4.0CC BY 4.0 Creative Commons Attribution 4.0 truetrue
Краткие подписи
Добавьте однострочное описание того, что собой представляет этот файл
NGC3190, a spiral galaxy of type SA(s)a in the constellation Leo, was imaged during engineering work at the KPNO Mayall 4-meter telescope in January of 2001.
Файл содержит дополнительные данные, обычно добавляемые цифровыми камерами или сканерами. Если файл после создания редактировался, то некоторые параметры могут не соответствовать текущему изображению.
Название изображения
NGC3190, a spiral galaxy of type SA(s)a in the constellation Leo, was imaged during engineering work at the KPNO Mayall 4-meter telescope in January of 2001. The large size of the telescope and the smaller format imager used for test work combine to make the field of view only just the size of the galaxy itself. Multiple exposures on this faint galaxy took a total of 3000s in the blue (B) band, 2000s in green (V) and 1000s in red (R). NGC3190 in fact forms a small group (Hickson 44, Arp 316) with NGC3193 to the east, NGC3187 to the west, and NGC3185, significantly further away to the southwest. Interestingly, NGC3189 refers to the south-west (lower right) part of NGC3190. The strong dust lane down the middle apparently misled the catalog compilers into giving it two separate numbers. NGC3190 also contains an active galactic nucleus.
Поставщик, кто предоставил изображение
Hillary Mathis/NOIRLab/NSF/AURA
Источник
NSF's NOIRLab
Краткое название
NGC 3190
Условия использования
Creative Commons Attribution 4.0 International License