[]
您当前的选择
资产 资产
您的报价 0

您的选择

清除选择
商品已加入购物车
{"event":"pageview","page_type1":"undetected","page_type2":"_assets_search_override","language":"cn","user_logged":"false","user_type":"ecommerce","nl_subscriber":"false"}
{"event":"ecommerce_event","event_name":"view_item","event_category":"browse_catalog","ecommerce":{"items":[{"item_id":"UIG867062","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"hidden_behind_a_shroud_of_dust_in_the_constellation_cygnus_is_an_exceptionally_bright_source_of_radi","item_variant":"undefined"},{"item_id":"UIG867060","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"hidden_behind_a_shroud_of_dust_in_the_constellation_cygnus_is_an_exceptionally_bright_source_of_radi","item_variant":"undefined"},{"item_id":"UIG867061","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"hidden_behind_a_shroud_of_dust_in_the_constellation_cygnus_is_an_exceptionally_bright_source_of_radi","item_variant":"undefined"},{"item_id":"PIX4621130","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"star_formation_in_the_dr21_region_star_formation_in_the_dr21_region_this_star_forming_region_is_abou","item_variant":"undefined"},{"item_id":"PIX4621115","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"star_formation_in_the_dr21_region_star_formation_in_the_dr21_region_this_star_formation_region_is_ab","item_variant":"undefined"},{"item_id":"UIS5104281","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"stellar_nursery_c_2005","item_variant":"undefined"}]}}
{"event":"custom_event","event_name":"view_search_result","event_category":"browse_catalog","keyword":"dr21","search_type":"standard","search_bridgeman_artists":"false","search_mode":"automatic","search_zero_result":"false","search_results":6,"search_results_page_number":1}

Dr21' 图片和/或视频结果 page 1 of 1

主要过滤器
购买印刷品选项
免版税选项
电子商务选项
路透社业绩
媒体类型
方向
颜色
权利类型
权利
更多过滤器
布里奇曼艺术家
布里奇曼摄影师
世纪
镜头滤镜
视频原始格式
视频分辨率
视频分类
Filter group
Filter colors
按以下排序:
每页
Filter group
权利类型
媒体类型
无版权
Filter colors

显示选项

View
Image Size

[2, 无限[找到'Dr21'的图片,6

Star Formation in the DR21 Region - Star Formation in the DR21 Region - This star-forming region is about 6200 years old - light. Hidden in light visible by interstellar dust, this region rises in infrared light. Gas filaments appear in red; they emphasize the presence of aromatic polycyclic hydrocarbons (PAH); they are organic molecules composed of carbon atoms and hydrogen that could be the germs on which the first bricks of life appeared. Image obtained by the Spitzer space telescope in 2003. Hidden behind a shroud of dust in the constellation Cygnus is a stellar nursery called DR21, which is giving birth to some of the most massive stars in our galaxy. Visible light images reveal no trace of this interstellar cauldron because of heavy dust obscuration. This image from Nasa's Spitzer Space Telescope allow us to peek behind the cosmic veil and pinpoint one of the most massive natal stars yet seen in our Milky Way galaxy. The never - before - seen star is 100,000 times as bright as the Sun. Also revealed for the first time is a powerful outflow of hot gas emanating from this star and bursting through a giant molecular cloud. The image is a large - scale mosaic assembled from individual photographs obtained with the Infraared Array Camera (IRAC) aboard Spitzer. The image covers an area about two times that of a full moon. The mosaic is a composite of images obtained at mid - infrared wavelengths of 3.6 microns (blue), 4.5 microns (green), 5.8 microns (orange) and 8 microns (red). The brightest infrared cloud near the top center corresponds to DR21, which presumably contains a cluster of newly forming stars at a distance of 10,000 light - years. Protruding out from DR21 toward the bottom left of the image is a gaseous outflow (green), containing both carbon monoxide and molecular hydrogen. Data from the Spitzer spectrograph, which breaks light into its constitutes
Star Formation in the DR21 Region - Star Formation in the DR21 Region - This star formation region is about 6200 years old - light. Hidden in light visible by interstellar dust, this region rises in infrared light. Gas filaments appear in red; they emphasize the presence of aromatic polycyclic hydrocarbons (PAH); they are organic molecules composed of carbon atoms and hydrogen that could be the germs on which the first bricks of life appeared. Composite image in different wavelengths obtained by the Spitzer space telescope; in blue the visible light, in yellow and red the infrared light. Hidden behind a shroud of dust in the constellation Cygnus is a stellar nursery called DR21, which is giving birth to some of the most massive stars in our galaxy. Visible light images reveal no trace of this interstellar cauldron because of heavy dust obscuration. This image from Nasa's Spitzer Space Telescope allow us to peek behind the cosmic veil and pinpoint one of the most massive natal stars yet seen in our Milky Way galaxy. The never - before - seen star is 100,000 times as bright as the Sun. Also revealed for the first time is a powerful outflow of hot gas emanating from this star and bursting through a giant molecular cloud. This colorful image is a large - scale composite mosaic assembled from data collected at a variety of different wavelengths. Views at visible wavelengths appear blue, near - infrared light is depicted as green, and mid - infrared data is portrayed as red. The result is a contrast between structures seen in visible light (blue) and those observed in the infrared (yellow and red). The image covers an area about two times that of a full moon. The red filaments stretching across the Spitzer image denote the presence of polycyclic aromatic hydrocarbons. These organic molecules, comprised of carbon and hydrogen, are excited by surrounding i
Stellar nursery, c 2005
内容合作伙伴限制
  • Not available to clients invoiced in the UK