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哈勃100622:N11,LMC中年轻巨星吹出的巨泡

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gohomeman1 发表于 2010-6-30 13:36 | 显示全部楼层 |阅读模式 来自: 浙江省宁波市 鄞州畅联信息技术有限公司

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http://www.spacetelescope.org/news/heic1011/

heic1011 - Photo Release,22 June 2010
哈勃欧洲信息中心2010年第11#新闻,图像类,2010.6.22公布
Hubble captures bubbles and baby stars
哈勃获得了年轻恒星和巨泡的照片


                               
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A spectacular new NASA/ESA Hubble Space Telescope image — one of the largest ever released of a star-forming region — highlights N11, part of a complex network of gas clouds and star clusters within our neighbouring galaxy, the Large Magellanic Cloud. This region of energetic star formation is one of the most active in the nearby Universe.
NASA、ESA合作的哈勃太空望远镜拍摄了N11 的特写,N11位于我们的伴星系——大麦哲伦星系(LMC)中,是最大的恒星诞生区之一,由复杂的气体云网和星团组成。这个剧烈的恒星诞生区是我们附近宇宙中最活跃的恒星孕育区之一。

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 楼主| gohomeman1 发表于 2010-6-30 13:44 | 显示全部楼层 来自: 浙江省宁波市 鄞州畅联信息技术有限公司
本帖最后由 gohomeman1 于 2010-8-10 00:54 编辑


                               
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http://www.spacetelescope.org/static/archives/images/original/heic1011a.tif,7546 x 7418,132.3MB

http://www.spacetelescope.org/static/archives/images/large/heic1011a.jpg,同上,28.1MB


The Large Magellanic Cloud contains many bright bubbles of glowing gas. One of the largest and most spectacular has the name LHA 120-N 11, from its listing in a catalogue compiled by the American astronomer and astronaut Karl Henize in 1956, and is informally known as N11. Close up, the billowing pink clouds of glowing gas make N11 resemble a puffy swirl of fairground candy floss. From further away, its distinctive overall shape led some observers to nickname it the Bean Nebula. The dramatic and colourful features visible in the nebula are the telltale signs of star formation. N11 is a well-studied region that extends over 1000 light-years. It is the second largest star-forming region within the Large Magellanic Cloud and has produced some of the most massive stars known.
大麦哲伦星系(LMC)包含许多明亮的发光气体云,其中最大、最著名的恒星诞生区之一,就是LHA 120-N11,它由美国天文学家兼宇航员尔.赫尼兹于1956年编纂,一般简称为N11。在特写画面中,翻涌的粉红色气体云看上去就像一大团集市中售卖的棉花糖。进一步的,因其奇特的外形,某些观测者昵称其为豆瓣星云。星云中这些壮观的特征是恒星正在形成的标志。 N11/已被广泛研究,它延展超过1000光年,是LMC中第二大的恒星孕育区,包含多个超大质量恒星。(最大的是蜘蛛星云——gohomeman1注)
It is the process of star formation that gives N11 its distinctive look. Three successive generations of stars, each of which formed further away from the centre of the nebula than the last, have created shells of gas and dust. These shells were blown away from the newborn stars in the turmoil of their energetic birth and early life, creating the ring shapes so prominent in this image.
N11因大量的恒星形成而与众不同。从中心开始,连续三代向外发展的恒星形成过程,构筑了N11星云的气体、尘埃外形。这些环状外形是新生恒星在其充满活力的婴幼儿期吹成的。
Beans are not the only terrestrial shapes to be found in this spectacular high resolution image from the NASA/ESA Hubble Space Telescope. In the upper left is the red bloom of nebula LHA 120-N 11A. Its rose-like petals of gas and dust are illuminated from within, thanks to the radiation from the massive hot stars at its centre. N11A is relatively compact and dense and is the site of the most recent burst of star development in the region.
在哈勃的高分辨图像中,我们不仅能看见地球上的“豆瓣”,在图像左上方还能看见“红花”:LHA120-N11 A。这朵玫瑰花般的气体尘埃云被其内部的热巨星辐射照亮。相对来说,N11 A更为致密,是最近才发展起来的星暴区域。(N11 A位置见4楼、16楼的图,本图中看不见——gohomeman1注)
Other star clusters abound in N11, including NGC 1761 at the bottom of the image, which is a group of massive hot young stars busily pouring intense ultraviolet radiation out into space. Although it is much smaller than our own galaxy, the Large Magellanic Cloud is a very vigorous region of star formation. Studying these stellar nurseries helps astronomers understand a lot more about how stars are born and their ultimate development and lifespan.
N11天区富含星团,比如图像下方的NGC 1761就是一个年轻的热巨星簇,正向宇宙中倾泻强烈的紫外辐射。虽然比银河系小得多,LMC却是一个充满活力的恒星诞生区。天文学家通过研究这些恒星孕育场所,能够更多地了解恒星是如何诞生的以及它们的最终演化历程。
Both the Large Magellanic Cloud and its small companion, the Small Magellanic Cloud, are easily seen with the unaided eye and have always been familiar to people living in the southern hemisphere. The credit for bringing these galaxies to the attention of Europeans is usually given to Portuguese explorer Fernando de Magellan and his crew, who viewed it on their 1519 sea voyage. However, the Persian astronomer Abd Al-Rahman Al Sufi and the Italian explorer Amerigo Vespucci recorded the Large Magellanic Cloud in 964 and 1503 respectively.
对南半球的居民来说,大麦哲伦星系(LMC)和它的伙伴小麦哲伦星系(SMC)能够方便地用肉眼看到,早已为他们所熟悉。但是,欧洲一般把这2个星系的发现者荣誉归于葡萄牙探险家费尔南多.麦哲伦和他的船队,认为是他们在1519年的环球航海中发现的。其实,早在公元964年、1503年,波斯天文学家Abd Al-Rahman Al Sufi和意大利探险家Amerigo Vespucci 就分别记录过它们。
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 楼主| gohomeman1 发表于 2010-6-30 13:49 | 显示全部楼层 来自: 浙江省宁波市 鄞州畅联信息技术有限公司
Notes 注释
The Hubble Space Telescope is a project of international cooperation between ESA and NASA.

哈勃望远镜是美国宇航局(NASA)和欧洲航天局(ESA)的国际间合作项目。
Image credit: NASA, ESA and Jesús Maíz Apellániz (Instituto de Astrofísica de Andalucía, Spain)
图像版权:美国宇航局、欧洲航天局,西班牙 安达卢西亚天体物理研究所的Jesús Maíz Apellániz

Links 链接 2010年发表的关于N11A的信息

Contacts
相关联系人
Colleen Sharkey
Hubble/ESA, Garching, Germany
德国加尔兴市,哈勃欧洲项目部
Tel: +49-89-3200-6306
Cell: +49-015115373591
Email: csharkey@eso.org
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 楼主| gohomeman1 发表于 2010-6-30 13:54 | 显示全部楼层 来自: 浙江省宁波市 鄞州畅联信息技术有限公司
本帖最后由 gohomeman1 于 2010-7-11 17:01 编辑

http://www.spacetelescope.org/images/heic1011b/

Overview of the Large Magellanic Cloud (annotated)
纵览大麦哲伦星系的一部分(带标注)


                               
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http://www.spacetelescope.org/static/archives/images/original/heic1011b.tif,3309 x 3316,23.2MB

http://www.spacetelescope.org/static/archives/images/large/heic1011b.jpg,同上,5.3MB

Location of the new Hubble image of the star forming region LHA 120-N 11. This image was created from digitised photographs through red and blue filters. The field of view is about three degrees across.
哈勃新拍摄的恒星诞生区——LHA120(即N11)所在的天区位置。本图宽约3度,根据DSS2中红、蓝光巡天数据创建。

Credit: ESO/Digitized Sky Survey 2.
版权:ESO,第2代 数字巡天项目(DSS2)
Acknowledgment: Davide De Martin
特别感谢:大卫.马丁
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 楼主| gohomeman1 发表于 2010-6-30 14:01 | 显示全部楼层 来自: 浙江省宁波市 鄞州畅联信息技术有限公司
本帖最后由 gohomeman1 于 2010-8-10 00:51 编辑

http://www.spacetelescope.org/images/heic1011c/

Overview of the Large Magellanic Cloud
纵览大麦哲伦星系的一部分


                               
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http://www.spacetele...l/heic1011c.tif,10643 x 10665,229.6MB

http://www.spacetele...e/heic1011c.jpg,同上,112.2MB

This wide field view of part of the Large Magellanic Cloud includes the location of the N11 star formation region. This image was created from digitised photographs through red and blue filters. The field of view is about three degrees across.
这张广域大图展示了大麦哲伦星系的一部分——N11恒星诞生区。本图宽约3度,根据 DSS2中红、蓝光巡天数据创建。

Credit: ESO/Digitized Sky Survey 2.
版权:ESO,第2代 数字巡天项目(DSS2)
Acknowledgment: Davide De Martin
特别感谢:大卫.马丁
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 楼主| gohomeman1 发表于 2010-6-30 14:16 | 显示全部楼层 来自: 浙江省宁波市 鄞州畅联信息技术有限公司
http://www.spacetelescope.org/images/heic1011d/

The entire Large Magellanic Cloud with annotations
带标注的大麦哲伦星系全图


                               
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http://www.spacetele...l/heic1011d.tif,5000 X 4105,172.3MB

http://www.spacetele...e/heic1011d.jpg,同上,13.1MB


This image shows the entire Large Magellanic Cloud, with some of the brightest objects marked. The outline shown corresponds to the overview image from Digitized Sky Survey 2. The field of view is about ten degrees across.
大麦哲伦星系全图,标注了其中最明亮的天体。其中的方框就是上一楼的DSS2大图所在。全图视场约10度宽。
Credit: Robert Gendler/ESO
版权:ESO,天文摄影大师Robert Gendler
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 楼主| gohomeman1 发表于 2010-6-30 17:51 | 显示全部楼层 来自: 浙江省宁波市 鄞州畅联信息技术有限公司
http://www.spacetelescope.org/news/heic0210/

heic0210 - Photo Release,12 September 2002
哈勃欧洲信息中心2002年第10
#新闻,图像类,2002.12.12公布
A rose blooming in space
怒放的宇宙玫瑰



                               
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Resembling a delicate rose floating in space, the nebula N11A is seen in a new light in a true-colour image taken by the NASA/ESA Hubble Space Telescope. Fierce radiation from massive stars embedded at the centre of N11A illuminates the surrounding gas with a soft fluorescent glow.
在哈勃太空望远镜拍摄的新彩图中,N11 A星云就像宇宙中一朵娇嫩的玫瑰。深嵌于星云中心的大质量巨星的强烈辐射激发星云气体发出柔弱的荧光。
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 楼主| gohomeman1 发表于 2010-6-30 18:09 | 显示全部楼层 来自: 浙江省宁波市 鄞州畅联信息技术有限公司
本帖最后由 gohomeman1 于 2010-6-30 18:14 编辑

http://www.spacetelescope.org/static/archives/images/pl_original/heic0210a.tif,7.6MB


                               
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什么垃圾版本啊,翻译的内容都丢失了!~现在IE发帖也有问题了?!

N11A is located in the constellation of Dorado (the Goldfish). This true-colour Hubble image is composed of three narrow-band filter images obtained with Hubble's Wide Field Planetary Camera 2 on 17 May 2000. The three images were obtained using a 1040 second exposure through a red filter (ionised hydrogen, H-alpha), a 1200 second exposure through a green filter (ionised oxygen), and a 1040 second exposure through a blue filter (ionised hydrogen, H-beta). N11A is about 10 arc-seconds in size, corresponding to about 8 light-years at the distance of the Large Magellanic Cloud (168 000 light-years).
N11 A位于剑鱼座的大麦哲伦星系,离我们约16.8万光年。本图由哈勃的第2代广域行星相机(WFPC2)摄于2002.5.17,三色合成的真彩色图。三个窄带滤光器的曝光时间为:
H-α,1040s,配色红;电离O,1200s,配色绿;H-β,1040s,配色蓝。N11 A的张角约10角秒,相当于8光年直径。
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人与自然 发表于 2010-7-1 22:48 | 显示全部楼层 来自: 广东省中山市 电信
大麦哲伦标注图收藏了,谢谢分享,辛苦了!
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麦香果奶 发表于 2010-7-9 12:37 | 显示全部楼层 来自: 福建省福州市 电信
提示: 作者被禁止或删除 内容自动屏蔽
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 楼主| gohomeman1 发表于 2010-7-10 01:02 | 显示全部楼层 来自: 浙江省宁波市 鄞州畅联信息技术有限公司
本帖最后由 gohomeman1 于 2010-7-10 01:26 编辑

http://hubblesite.org/newscenter/archive/releases/2004/22/

July 1, 2004  09:00 AM (EDT)
News Release Number: STScI-2004-22
太空望远镜科研所2004年第22#新闻公报,美国东部时间2004.7.1 09:00公布。

Hubble Studies Generations of Star Formation in Neighboring Galaxy
哈勃在邻近星系研究恒星诞生区的世代关系


                               
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July 1, 2004: NASA's Hubble Space Telescope captures the iridescent tapestry of star birth in a neighboring galaxy in this panoramic view of glowing gas, dark dust clouds, and young, hot stars. The star-forming region, catalogued as N11B, lies in the Large Magellanic Cloud (LMC), located only 160,000 light-years from Earth. With its high resolution, the Hubble Space Telescope is able to view details of star formation in the LMC as easily as ground-based telescopes are able to observe stellar formation within our own Milky Way galaxy.
2004.7.1:哈勃太空望远镜在邻近星系中拍摄了一个恒星诞生区的全景图,云锦般的图像中充满发光气体、暗尘埃云和年轻的热巨星。这个恒星诞生区编号为N11B,位于大麦哲伦星系(LMC),离地球约16万光年。基于哈勃的高分辨率,研究其中的细节与通过地面望远镜研究银河系中恒星孕育区一样容易。
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 楼主| gohomeman1 发表于 2010-7-10 01:05 | 显示全部楼层 来自: 浙江省宁波市 鄞州畅联信息技术有限公司
本帖最后由 gohomeman1 于 2010-7-11 17:12 编辑

http://hubblesite.org/newscenter/archive/releases/2004/22/image/a/


                               
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http://imgsrc.hubblesite.org/hu/db/images/hs-2004-22-a-full_tif.tif,1.8MB

ABOUT THIS IMAGE:
NASA's Hubble Space Telescope captures this iridescent tapestry of star birth in a neighboring galaxy in this panoramic view of glowing gas, dark dust clouds, and young, hot stars. The star-forming region, catalogued as N11B, lies in the Large Magellanic Cloud (LMC), located only 160,000 light-years from Earth. With its high resolution, the Hubble Space Telescope is able to view details of star formation in the LMC as easily as ground-based telescopes are able to observe stellar formation within our own Milky Way galaxy. This new Hubble image zooms in on N11B, which is a small subsection within an area of star formation cataloged as N11. N11 is the second largest star-forming region in the LMC. Within the LMC, N11 is surpassed in size and activity only by the immense Tarantula nebula (also known as 30 Doradus.)
NASA的哈勃太空望远镜在邻近星系中拍摄了一个恒星诞生区的全景图,云锦般的图像中充满发光气体、暗尘埃云和年轻的热巨星。这个恒星诞生区编号为N11B,位于大麦哲伦星系(LMC),离地球约 16万光年。基于哈勃的高分辨率,研究其中的细节与通过地面望远镜研究银河系中恒星孕育区一样容易。这张哈勃的新图放大了N11B中的细节,它仅是N11整个区域的一小部分。在LMC中,N11是第2大的恒星孕育区,尺度和活跃度仅次于最出色的蜘蛛星云(又名剑鱼座30)。
The image illustrates a perfect case of sequential star formation in a nearby galaxy where new star birth is being triggered by previous-generation massive stars. A collection of blue- and white-colored stars near the left of the image are among the most massive stars known anywhere in the universe. The region around the cluster of hot stars in the image is relatively clear of gas, because the stellar winds and radiation from the stars have pushed the gas away. When this gas collides with and compresses surrounding dense clouds, the clouds can collapse under their own gravity and start to form new stars. The cluster of new stars in N11B may have been formed this way, as it is located on the rim of the large, central interstellar bubble of the N11 complex. The stars in N11B are now beginning to clear away their natal cloud, and are carving new bubbles in turn. Yet another new generation of stars is now being born in N11B, inside the dark dust clouds in the center and right-hand side of the Hubble image. This chain of consecutive star birth episodes has been seen in more distant galaxies, but it is shown very clearly in this new Hubble image.
本图完美诠释了邻近星系的恒星诞生区中,上一代大质量恒星是如此触发下一代恒星诞生的。图像左方的蓝白色星团中充斥着宇宙中到处可见的蓝超巨星,星团周围区域,因炽热巨星的强烈辐射和强劲恒星风,气体基本都被吹跑了。这些吹散的气体与更远处的气体相互作用,压缩了气体云并引发了它们的引力坍缩过程,形成新一代恒星。在N11B中心附近复杂的空腔壁上,新一代恒星很可能就是以这种方式形成的。新生的恒星正在清除其周围的襁褓气体,形成新的空泡。在图中央和右方的黑暗尘埃云中,更新一代的恒星正在形成。这种持续的恒星诞生链可以在非常遥远的星系中看到,但现在清晰展示在这张哈勃的新图像中。
Farther to the right of the image, along the top edge, are several smaller dark clouds of interstellar dust with odd and intriguing shapes. They are seen silhouetted against the glowing interstellar gas. Several of these dark clouds are bright-rimmed because they are illuminated and are being evaporated by radiation from neighboring hot stars.
在图的右上方,我们可以看到一些有着奇特外形的暗星云,它们是在发光星际云前的稠密星际尘埃。其中的一些暗云有着发光的镶边,因为它们内蕴的新生灼热恒星正在照亮并蒸发它们。
This image was taken with Hubble's Wide Field Planetary Camera 2 using filters that isolate light emitted by hydrogen and oxygen gas. The science team, led by astronomers You-Hua Chu (University of Illinois) and Yäel Nazé (Universite de Liège, Belgium) are comparing these images of N11B, taken in 1999, with similar regions elsewhere in the LMC. This color composite image was co-produced and is being co-released by the Hubble Heritage Team (STScI) and the Hubble European Space Agency Information Center (HEIC).
本图由哈勃的第二代广域行星相机(WFPC2)拍摄于1999年,滤光器对应氢和氧的发射线。由伊利诺伊大学楚友华(音)和比利时列日大学 Y. Nazé 牵头的科学家团队,比较了N11与LMC中类似区域的图像。这张彩色合成图像由哈勃遗产团队和欧洲空间局哈勃信息中心(HEIC)联合制作、发布。

Object Name: N11B
对象名称:N11B
Image Type: Astronomical
图像类型:天体
Image Credit: NASA, ESA, and The Hubble Heritage Team (AURA/STScI)
版权:NASA、ESA,哈勃遗产团队(太空望远镜科研所/美国大学天文研究联合会)
Acknowledgment: Y.-H. Chu (U. Illinois, Urbana-Champaign) and Y. Nazé (U. Liège, Belgium)
特别感谢:美国伊利诺伊大学厄巴纳-香槟分校(或平原大学) 楚友华(音),比利时列日大学 Y. Nazé  
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 楼主| gohomeman1 发表于 2010-7-10 01:21 | 显示全部楼层 来自: 浙江省宁波市 鄞州畅联信息技术有限公司
本帖最后由 gohomeman1 于 2010-7-11 17:10 编辑

http://hubblesite.org/newscenter/archive/releases/2004/22/image/b/

N11, the Second-Largest Star Formation Region in the Large Magellanic Cloud
N11,大麦哲伦星系中第2大的恒星诞生区


                               
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http://imgsrc.hubblesite.org/hu/db/images/hs-2004-22-b-full_tif.tif,6.4MB

曲尺形图像是WFPC2的标准特征。同样的文字就不翻译了。

Object Name: N11B
对象名称:N11B
Image Type: Astronomical
图像类型:天体
Image Credit: NASA, ESA, and The Hubble Heritage Team (AURA/STScI)
版权:NASA、ESA,哈勃遗产团队(太空望远镜科研所/美国大学天文研究联合会)
Acknowledgment: Y.-H. Chu (U. Illinois, Urbana-Champaign) and Y. Nazé (U. Liège, Belgium)
特别感谢:美国伊利诺伊大学厄巴纳 -香槟分校(或平原大学) 楚友华(音),比利时列日大学 Y. Nazé
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 楼主| gohomeman1 发表于 2010-7-10 01:23 | 显示全部楼层 来自: 浙江省宁波市 鄞州畅联信息技术有限公司
http://hubblesite.org/newscenter/archive/releases/2004/22/fastfacts/

Technical facts about this news release:

About the Object
Object Name:N11B
Object Description:H II Region in the LMC
Position (J2000):R.A. 4h 56m 51s.96
Dec. -66° 24' 32".01
Constellation:Dorado
Distance:Approximately 160,000 light-years (50 kiloparsecs)
Dimensions:This image is roughly 2.2 arcminutes (105 light-years or 32 parsecs) wide.
About the Data
Data Description:This image was created from HST data from the following proposal: 6698: Y.-H. Chu (U. Illinois at Urbana - Champaign), D. Bomans and K. Weis (Universitat Bochum), G. Garcia-Segura and M. Rosado (UNAM), A. Laval (Observatoire de Marseille), S. Points (Northwestern U.), H. Yang (U. Minnesota - Twin Cities) Y. Naze (Universite de Liege, Belgium) is also a science collaborator.
Instrument:WFPC2
Exposure Date(s):May 12, 1999
Exposure Time:37 minutes
Filters:F656N (Halpha), F502N ([O III])
About the Image
Image Credit:NASA, ESA, The Hubble Heritage Team (STScI/AURA) and HEIC
Release Date:July 1, 2004
Orientation:
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 楼主| gohomeman1 发表于 2010-7-10 01:23 | 显示全部楼层 来自: 浙江省宁波市 鄞州畅联信息技术有限公司
本帖最后由 gohomeman1 于 2010-7-11 20:40 编辑


                               
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Technical facts about this image:
图像科学数据

About  the Object
关于天体  
Object Name:  N11B
对象名称: N11B
Object Description:  H II Region in the LMC
对象类型:大麦哲伦星系(LMC)中的电离氢区(HⅡ)
Position (J2000):     4h 56m 51s.96    Dec. -66° 24' 32".01
坐标(儒略纪元2000星历表): 赤经 4时56分51.96秒,赤纬 -66°24′32.01″
Constellation:  Dorado
星座:剑鱼座
Distance: Approximately 160,000 light-years (50 kiloparsecs).
距离:约16万光年,5万秒差距
Dimensions:   This image is roughly 2.2 arcminutes (105 light-years or 32 parsecs) wide.
图像尺寸:约2.2角分,或者说是105光年、32秒差距。

About  the Data
数据相关
Data Description:  The image was created from Hubble data from proposal 6698: Y.-H. Chu (U. Illinois at Urbana - Champaign), D. Bomans and K. Weis (Universitat Bochum), G. Garcia-Segura and M. Rosado (UNAM), A. Laval (Observatoire de Marseille), S. Points (Northwestern U.), H. Yang (U. Minnesota - Twin Cities) Y. Naze (Universite de Liege, Belgium) is also a science collaborator.
数据说明:本图根据第6698#申请的哈勃数据库数据创建,申请团队包括:
美国伊利诺伊大学厄巴纳 -香槟分校 楚友华(音);
德国 波鸿大学  D. Bomans、K. Weis;
墨西哥国立自治大学(UNAM)  D. Bomans、K. Weis;
马赛天文台 A. Laval; 美国西北大学 S. Points;
明尼苏达大学双城分校 H. Yang;比利时列日大学 Y. Nazé等。
Instrument:  WFPC2
仪器:第二代广域行星相机(WFPC2)
Exposure Date(s):  May 12, 1999
拍摄日期:1999.5.12
Exposure Time: 37 minutes
曝光时间: 37分钟
Filters: F656N (Halpha), F502N ([O III])
滤光器:656nm的氢H-α线,502nm的电离氧[OⅢ]。

About  the Image
关于公布图像
Image Credit: NASA, ESA, The Hubble Heritage Team (STScI/AURA)
版权:美国宇航局,欧洲空间局;哈勃遗产团队(太空望远镜科研所/ 美国大学天文研究联合会)。
Release Date: July 1, 2004
公布日期:2004.7.1
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 楼主| gohomeman1 发表于 2010-7-10 01:25 | 显示全部楼层 来自: 浙江省宁波市 鄞州畅联信息技术有限公司
本帖最后由 gohomeman1 于 2010-7-11 17:27 编辑

http://hubblesite.org/newscenter/archive/releases/2004/22/image/c/

Ground-Based Image of LMC N11
N11的地面望远镜图像

                               
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http://imgsrc.hubblesite.org/hu/db/images/hs-2004-22-c-full_tif.tif,2.8MB

ABOUT THIS IMAGE:
An image of N11 in the Large Magellanic Cloud, taken with the Curtis Schmidt telescope at Cerro Tololo Interamerican Observatory (CTIO) as part of the Magellanic Clouds Emission-Line Survey (MCELS). These data were taken by CTIO astronomical observers, Claudio Aguilera, Sean Points, and Chris Smith, who is also the lead investigator of the MCELS project.
由托洛洛山美洲天文台(CTIO)上的柯蒂斯.施密特望远镜拍摄的N11图像,它是麦哲伦星系发射线巡天(MCELS)图像的一部分。这些数据来自CTIO天文观测者 Claudio Aguilera, Sean Points 和 Chris Smith,他们是MCELS项目的主要研究者。
This color image was produced using three separate exposures taken in hydrogen, sulfur and oxygen bandpasses.
本图是三色合成的,对应氢、硫和氧的发射线。

Object Name: N11
对象名称:N11
Image Type: Astronomical
图像类型:天体
Photo Credit: NASA; C. Aguilera, S. Points, and C. Smith (CTIO); and Z. Levay (STScI)
照片版权:NASA,太空望远镜科研所 Z. Levay;托洛洛山美洲天文台(CTIO) C. Aguilera, S. Points, C. Smith
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altmis 发表于 2010-7-10 15:35 | 显示全部楼层 来自: 上海市 电信
好多好多星星哦 ::0022::
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李乾坤 发表于 2016-7-1 09:04 | 显示全部楼层 来自: 黑龙江省哈尔滨市 电信
这是真能吹,吹这么大。
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李乾坤 发表于 2017-1-13 08:05 | 显示全部楼层 来自: 黑龙江省哈尔滨市 电信
转眼6年多了。
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