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ESO110824:VST拍摄美丽的“室女座之眼”星系

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叶程婉 发表于 2011-8-27 07:35 | 显示全部楼层 |阅读模式 来自: 中国–广东–佛山–顺德区 电信

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http://www.eso.org/public/news/eso1131/
VLT Looks into The Eyes of the Virgin

                               
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ESO’s Very Large Telescope has taken a striking image of a beautiful yet peculiar pair of galaxies nicknamed The Eyes. The larger of these, NGC 4438, was once a spiral galaxy but has become badly deformed by collisions with other galaxies in the last few hundred million years. This picture is the first to come out of ESO’s Cosmic Gems programme, an initiative in which ESO has granted dedicated observing time for outreach purposes.

The Eyes are about 50 million light-years away in the constellation of Virgo (The Virgin) and are some 100 000 light-years apart. The nickname comes from the apparent similarity between the cores of this pair of galaxies — two white ovals that resemble a pair of eyes glowing in the dark when seen in a moderate-sized telescope.

But although the centres of these two galaxies look similar, their outskirts could not be more different. The galaxy in the lower right, known as NGC 4435, is compact and seems to be almost devoid of gas and dust. In contrast, in the large galaxy in the upper left (NGC 4438) a lane of obscuring dust is visible just below its nucleus, young stars can be seen left of its centre, and gas extends at least up to the edges of the image.

The contents of NGC 4438 have been stripped out by a violent process: a collision with another galaxy. This clash has distorted the galaxy’s spiral shape, much as could happen to the Milky Way when it collides with its neighbouring galaxy Andromeda in three or four billion years.

NGC 4435 could be the culprit. Some astronomers believe that the damage caused to NGC 4438 resulted from an approach between the two galaxies to within about 16 000 light-years that happened some 100 million years ago. But while the larger galaxy was damaged, the smaller one was significantly more affected by the collision. Gravitational tides from this clash are probably responsible for ripping away the contents of NGC 4438, and for reducing NGC 4435’s mass and removing most of its gas and dust.

Another possibility is that the giant elliptical galaxy Messier 86, further away from The Eyes and not visible in this image, was responsible for the damage caused to NGC 4438. Recent observations have found filaments of ionised hydrogen gas connecting the two large galaxies, indicating that they may have collided in the past.

The elliptical galaxy Messier 86 and The Eyes belong to the Virgo Cluster, a very rich grouping of galaxies. In such close quarters, galaxy collisions are fairly frequent, so perhaps NGC 4438 suffered from encounters with both NGC 4435 and Messier 86.

This picture is the first to be produced as part of the ESO Cosmic Gems programme. This is a new initiative to produce astronomical images for educational and public outreach purposes. The programme mainly makes use of time when the sky conditions are not suitable for science observations to take pictures of interesting, intriguing or visually attractive objects. The data are also made available to professional astronomers through ESO’s science archive.

In this case, although there were some clouds, the atmosphere was exceptionally stable, which allowed very sharp details to be revealed in this image taken using the VLT’s FORS2 [1] instrument. Light passing through two different filters was used: red (coloured red) and green-yellow (coloured blue), and the exposure times were 1800 seconds and 1980 seconds, respectively.
Notes

[1] FORS2 is the visual and near ultraviolet FOcal Reducer and low dispersion Spectrograph for the VLT. It is installed on the VLT’s Unit Telescope 1.
More information

ESO, the European Southern Observatory, is the foremost intergovernmental astronomy organisation in Europe and the world’s most productive astronomical observatory. It is supported by 15 countries: Austria, Belgium, Brazil, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world’s most advanced visible-light astronomical observatory and two survey telescopes. VISTA works in the infrared and is the world’s largest survey telescope and the VLT Survey Telescope is the largest telescope designed to exclusively survey the skies in visible light. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning a 40-metre-class European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become “the world’s biggest eye on the sky”.
Links

    ESO’s Cosmic Gems Programme
    Photos of the VLT

Contacts

Richard Hook
ESO, La Silla, Paranal, E-ELT and Survey Telescopes Public Information Officer
Garching bei München, Germany
Tel: +49 89 3200 6655
Email: rhook@eso.org

Olivier R. Hainaut
ESO, Science Liaison, education and Public Outreach Department
Garching bei München, Germany
Tel: +49 89 3200 6752
Cell: +49 151 2262 0554
Email: ohainaut@eso.org

Lars Lindberg Christensen
Head, ESO education and Public Outreach Department
Garching bei München, Germany
Tel: +49-89-3200-6761
Cell: +49-173-3872-621
Email: lars@eso.org
 楼主| 叶程婉 发表于 2011-8-27 07:38 | 显示全部楼层 来自: 中国–广东–佛山–顺德区 电信
欧洲南方天文台拍摄美丽“室女座之眼”星系
http://tech.qq.com/a/20110827/000067.htm
中文翻译引自 <中国天文科普网>
[导读]组成“室女座之眼”的两个星系位于50000万光年之遥的室女座,它们的昵称来自这对星系的核心——当我们通过中等望远镜看去,它们看上去就像黑暗中的一对眼睛。
“室女座之眼”位于室女座,离我们约5000万光年,两个星系之间距离约10万光年。它们的昵称来自这对星系的核心——当我们通过中等望远镜看去,它们看上去就像黑暗中的一对眼睛。

虽然这对星系的核心相似,它们的外围明显不同。位于右下的NGC 4435,看来比较致密,缺少气体和尘埃;而位于左上的大星系NGC 4438,在核心前横着一条尘埃带,左边还有年轻恒星群,气体更是延伸到图像的左右边缘。

NGC 4438与另一个星系的强烈相互作用使其外围剥离:冲突扭曲了星系的外形。当30~40亿年后银河系与仙女座大星系相遇时,会发生类似的过程。
NGC 4435就是罪魁祸首。有的天文学家相信,这些破坏是大约一亿年前,它与NGC 4438以1.6万光年近距离擦过造成的。但是随着大星系的外形被破坏,较小的NGC 4435会受到更大的影响。潮汐力既然能把NGC 4438的内容物扯出来,也能剥离NGC 4435的大部分气体、尘埃,减少星系的总质量。

另一种可能是更远的巨椭圆星系M 86(未在图中显示)的强大引力,造成了NGC 4438的形状改变。最新的观测显示,这两个大星系之间存在电离氢的纤维桥,意味着它们在过去发生过冲突。

巨椭圆星系M 86和NGC 4438、4435都属于室女座星系团,这是一个富含星系的集团。在这种环境中,星系相撞是非常常见的,因此NGC 4438很可能与这两者都遭遇过。

本图是“ESO宇宙珍宝节目”(ESO Cosmic Gems programme)的首个图像,这是ESO为公共教育和宣传而设立的新项目,主要在天空状况不适合进行科学观测的时候,就让仪器拍摄那些有趣的、有魅力的天体。这些数据同样可以用于专业天文学家的科学研究。

                               
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gohomeman1 发表于 2011-8-27 08:33 | 显示全部楼层 来自: 中国–浙江–宁波 电信
喂,你这样不好吧,既然copy的是我的翻译,怎么又写着腾讯的链接呢!
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 楼主| 叶程婉 发表于 2011-8-27 08:36 | 显示全部楼层 来自: LAN
发帖子之前我还在坛子里找了一圈,不过没找到您的翻译,那腾讯的链接上面就是写的从中国天文科普网转载的。
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gohomeman1 发表于 2011-8-27 08:40 | 显示全部楼层 来自: 中国–浙江–宁波 电信
回复 4# 叶程婉

呵呵,看来腾讯确实够快的:
http://www.astron.ac.cn/bencandy-3-5564-1.htm

最近一个月都很忙,只能给出这样的翻译,发帖肯定要拖延一段时间了
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