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GRE閱讀高頻機(jī)經(jīng)原文：藍(lán)脫序星的兩種形成過程

藍(lán)脫序星blue straggler的兩種形成過程

Vampires and collisions rejuvenate stars

Using the NASA/ESA Hubble Space Telescope, astronomers have uncovered two distinct kinds of "rejuvenated" stars in the globular cluster Messier 30. A new study shows that both stellar collisions and a process sometimes called vampirism are behind this cosmic "face lift". The scientists also uncover evidence that both sorts of blue stragglers were produced during a critical dynamical event (known as "core collapse") that occurred in Messier 30 a few billion years ago.

Stars in globular clusters [1] are generally extremely old, with ages of 12-13 billion years. However, a small fraction of them appear to be significantly younger than the average population and, because they seem to have been left behind by the stars that followed the normal path of stellar evolution and became red giants, have been dubbed blue stragglers [2]. Blue stragglers appear to regress from "old age" back to a hotter and brighter "youth", gaining a new lease on life in the process. A team of astronomers used Hubble to study the blue straggler star content in Messier 30, which formed 13 billion years ago and was discovered in 1764 by Charles Messier. Located about 28 000 light-years away from Earth, this globular cluster — a swarm of several hundred thousand stars — is about 90 light-years across.

Although blue stragglers have been known since the early 1950s, their formation process is still an unsolved puzzle in astrophysics. "It’s like seeing a few kids in the group picture of a rest-home for retired people. It is natural to wonder why they are there," says Francesco Ferraro from the University of Bologna in Italy, lead author of the study that will be published this week in Nature [3]. Researchers have been studying these stars for many years and knew that blue stragglers are indeed old. They were thought to have arisen in a tight binary system [4]. In such a pair, the less massive star acts as a "vampire", siphoning fresh hydrogen from its more massive companion star. The new fuel supply allows the smaller star to heat up, growing bluer and hotter — behaving like a star at an earlier stage in its evolution.

The new study shows that some of the blue stragglers have instead been rejuvenated by a sort of "cosmic facelift", courtesy of cosmic collisions. These stellar encounters are nearly head-on collisions in which the stars might actually merge, mixing their nuclear fuel and re-stoking the fires of nuclear fusion. Merged stars and binary systems would both be about twice the typical mass of individual stars in the cluster.

"Our observations demonstrate that blue stragglers formed by collisions have slightly different properties from those formed by vampirism. This provides a direct demonstration that the two formation scenarios are valid and that they are both operating simultaneously in this cluster," says team member Giacomo Beccari from ESA.

Using data from the now-retired Wide Field Planetary Camera 2 (WFPC2) aboard Hubble, astronomers found that these "straggling" stars are much more concentrated towards the centre of the cluster than the average star. "This indicates that blue stragglers are more massive than the average star in this cluster," says Ferraro. "More massive stars tend to sink deep into the cluster the way a billiard ball would sink in a bucket of honey."

The central regions of high density globular clusters are crowded neighbourhoods where interactions between stars are nearly inevitable. Researchers conjecture that one or two billion years ago, Messier 30 underwent a major "core collapse" that started to throw stars towards the centre of the cluster, leading to a rapid increase in the density of stars. This event significantly increased the number of collisions among stars, and favoured the formation of one of the families of blue stragglers. On the other hand, the increase of stellar crowding due to the collapse of the core also perturbed the twin systems, encouraging the vampirism phenomenon and thus forming the other family of blue stragglers. "Almost ten percent of galactic globular clusters have experienced core collapse, but this is the first time that we see the effect of the core collapse imprinted on a stellar population," says Barbara Lanzoni, University of Bologna.

"The two distinct populations of blue stragglers discovered in Messier 30 are the relics of the collapse of the core that occurred two billion years ago. In a broad context our discovery is direct evidence of the impact of star cluster dynamics on stellar evolution. We should now try to see if other globular clusters present this double population of blue stragglers," concludes Ferraro.

GRE閱讀詞匯精選之滲透

douse　v.把…浸入水中，用水潑

drenched　adj.濕透的

soak　v.浸泡，滲透

soaked　adj.濕透的

sodden　adj.浸透了的

soggy　adj.濕透的，濡濕的

souse　v.浸在水中，使?jié)裢?/p>

steep　v.浸泡，浸透

logged　adj　笨重的，濕透的

immerse　v.浸入，沉浸于

immersion　n.沉入，浸入

macerate　v.浸軟，消瘦

GRE閱讀表示選擇的邏輯詞匯總

邏輯

詞條

詞性

例句

選擇

otherwise

adv.

You need to work hard. Otherwise, you will fail.

選擇

or (else)

conj.

You need to work hard, or (else) you will fail.

選擇

lest

conj.

You need to work hard, lest you fail the exam.

選擇

in case

conj.

You need to work hard, in case the exam is hard.

GRE閱讀表示轉(zhuǎn)折的邏輯詞匯總

邏輯

詞條

詞性

例句

轉(zhuǎn)折

but

conj.

I worked hard, but I failed.

轉(zhuǎn)折

however

adv.

I worked hard. However, I failed.

轉(zhuǎn)折

nevertheless

adv.

I worked hard. Nevertheless, I failed.

轉(zhuǎn)折

still

adv.

I worked hard. Still, I failed.

轉(zhuǎn)折

nonetheless

adv.

I worked hard. Nonetheless, I failed.

轉(zhuǎn)折

though

adv.

I worked hard. I failed, though.

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