Gas, dust and stars: the life cycle of galaxies

气体、尘埃和恒星：星系的生命周期

• 批准号: ST/F003196/1
• 负责人: Albert Zijlstra
• 金额: $ 258.05万
• 依托单位: University of Manchester
• 依托单位国家: 英国
• 项目类别: Research Grant
• 财政年份: 2008
• 资助国家: 英国
• 起止时间: 2008 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=ST%2FF003196%2F1
• 关键词: Gas; dust; stars; life; cycle

The Universe is in constant evolution. Stars form out of clouds of gas. They live by burning hydrogen into helium, and later into carbon and oxygen. The nuclear burning takes place in the centre of the stars, but the products are brought to the surface and change the composition of the star. At the end of its life, the star will expel half or more of its mass in a catastrophic wind. The material blown off from these evolved stars forms fantastic and beautiful structures (e.g. Planetary Nebulae), we don't fully understand the physics that generates the structures but suspect that binary systems and magnetic fields are a factor. The wind expels the newly formed elements into space where they enrich clouds of gas. Thus, the next generation of stars will benefit from these new elements. At the same time, some elements condense as small particles, forming dust grains. These grains are also added to the clouds. When new stars form from this cloud, some of this dust will start the formation of planets. We are studying this cycle of evolution of stars, dust and gas. We study the input of new dust into the interstellar medium, looking at a variety of objects, with special emphasis on conditions of low metallicity, as existed in the early Universe. We study how stars form, especially stars more massive than the Sun. We look at the properties of dust over a complete galaxy (the Large Magelanic Cloud is the main target). We also study the chemistry of interstellar and circumstellar gas. We are also trying to understand how the presence of binary systems can affect the physics of the mass-loss process. The solar system is itself the result of this Universe of evolution. Dust left over from its formation is still present, incorporated in large grains or even comets and meteorites. Space craft are now collecting this dust. One of the goals of our research is to find the progeny of the proto-solar dust, among the outflows of other stars.

宇宙在不断地演化。恒星是由气体云形成的。它们靠将氢燃烧成氦，再燃烧成碳和氧而生存。核燃烧发生在恒星的中心，但产物被带到表面，改变了星星的组成。在它生命的尽头，星星将以灾难性的风的形式排出一半或更多的质量。从这些演化的恒星中吹出的物质形成了奇妙而美丽的结构（例如行星状星云），我们并不完全了解产生这些结构的物理学，但怀疑双星系统和磁场是一个因素。风将新形成的元素驱逐到太空中，在那里它们丰富了气体云。因此，下一代恒星将受益于这些新元素。与此同时，一些元素凝结成小颗粒，形成尘埃颗粒。这些颗粒也被添加到云中。当新的恒星从这片星云中形成时，其中的一些尘埃将开始形成行星。我们正在研究恒星、尘埃和气体的演化周期。我们研究新的尘埃进入星际介质的输入，在各种各样的对象，特别强调低金属量的条件，存在于早期宇宙。我们研究恒星是如何形成的，特别是比太阳质量更大的恒星。我们研究了整个星系上尘埃的性质（大麦哲伦星云是主要目标）。我们还研究星际和星周气体的化学。我们还试图了解二元系统的存在如何影响质量损失过程的物理学。太阳系本身就是这个宇宙进化的结果。它形成时留下的尘埃仍然存在，合并成大颗粒，甚至彗星和陨石。太空船正在收集这些尘埃。我们研究的目标之一是在其他恒星的外流中找到原太阳尘埃的后代。

项目成果

THE DETECTION OF INFRARED SiS BANDS IN SPECTRA OF S STARS

S星光谱中红外SiS波段的检测

• DOI: 10.1088/0004-637x/690/2/l122
• 发表时间: 2009
• 期刊: The Astrophysical Journal
• 作者: Cami J

Cold dust in three massive evolved stars in the LMC

LMC 中三颗巨大演化恒星中的冷尘埃

• DOI: 10.1051/0004-6361/201014513
• 发表时间: 2010
• 期刊: Astronomy and Astrophysics
• 影响因子: 6.5
• 作者: Boyer M

Dissection of the protostellar envelope surrounding IRAS 05173-0555 in L1634

L1634 中 IRAS 05173-0555 周围原恒星包膜的解剖

• DOI: 10.1051/0004-6361-20079224
• 发表时间: 2008
• 期刊: ASTRONOMY & ASTROPHYSICS
• 影响因子: 6.5
• 作者: Beltran M. T.

SPITZER SURVEY OF THE LARGE MAGELLANIC CLOUD, SURVEYING THE AGENTS OF A GALAXY'S EVOLUTION (SAGE). IV. DUST PROPERTIES IN THE INTERSTELLAR MEDIUM

• DOI: 10.1088/0004-6256/136/3/919
• 发表时间: 2005-06
• 期刊: The Astronomical Journal
• 作者: M. Meixner;K. Gordon;R. Indebetouw;J. Hora;B. Whitney;R. Blum;W. Reach;J. Bernard;M. Meade;B. Babler;C. Engelbracht;B. For;K. Misselt;U. Vijh;C. Leitherer;M. Cohen;E. Churchwell;F. Boulanger;J. Frogel;Y. Fukui;J. Gallagher;V. Gorjian;J. Harris;D. Kelly;A. Kawamura;Soyoung Kim;W. Latter;S. Madden;Ciska Markwick-Kemper;A. Mizuno;N. Mizuno;J. Mould;A. Nota;M. Oey;K. Olsen;T. Onishi;R. Paladini;N. Panagia;P. Pérez-González;H. Shibai;Sato Shuji;Linda J. Smith;L. Staveley-Smith;A. Tielens;T. Ueta;S. V. Dyk;K. Volk;M. Werner;D. Zaritsky

The JCMT Legacy Survey of the Gould Belt: a first look at Orion B with HARP

• DOI: 10.1111/j.1365-2966.2009.15619.x
• 发表时间: 2009-08
• 期刊: Monthly Notices of the Royal Astronomical Society
• 影响因子: 4.8
• 作者: J. Buckle;E. Curtis;J. Roberts;G. White;G. White;J. Hatchell;C. Brunt;H. Butner;B. Cavanagh-B.-Cav