Glistening galaxies tend to cluster in busiest parts of universe

Washington, May 20 (ANI): Glistening galaxies preferentially occupy regions of the universe containing more dark matter, astronomers have found.

Using a super-sensitive camera/spectrometer on the Herschel Space
Observatory, astronomers, including a UC Irvine team led by Asantha
Cooray, have mapped the skies as they appeared 10 billion years ago.

The UCI scientists found that these glistening galaxies preferentially occupy regions of the universe containing more dark matter and that collisions probably caused the abundant star production.

Cooray, associate professor and Chancellor”s Fellow in physics & astronomy, said: “Thanks to the superb resolution and sensitivity of the SPIRE [Spectral & Photometric Imaging Receiver] instrument on Herschel, we managed to map in detail the spatial distribution of massively star-forming galaxies in the early universe.

“All indications are that these galaxies are…crashing, merging, and possibly settling down at centers of large dark-matter halos.”

This information will enable scientists to adapt conventional theories of galaxy formation to accommodate the strange, star-filled versions.

The European Space Agency”s Herschel observatory carries the largest astronomical telescope operating in space today; it collects data at far-infrared wavelengths invisible to the naked eye.

One of three cameras on Herschel, SPIRE has let Cooray and colleagues survey large areas of the sky – about 60 times the size of the full Moon – in the constellations of Ursa Major and Draco.

The data analysed in this study was among the first to come from the Herschel Multi-Tiered Extragalactic Survey, the space observatory”s largest project. UCI is one of only four U.S. educational institutions involved in Herschel using the SPIRE instrument.

Seb Oliver, a University of Sussex professor who leads the survey, said: “It”s just the kind of thing we were hoping for from Herschel…and was only possible because we can see so many thousands of galaxies. It will certainly give the theoreticians something to chew over.”

The study will be published in a special issue of Astronomy & Astrophysics dedicated to the first scientific results from Herschel. (ANI)

Stars become overweight due to ‘stellar cannibalism’

London, Jan 15 (ANI): In a new research, scientists have discovered that the mysterious overweight stars known as blue stragglers are the result of ‘stellar cannibalism’ where plasma is gradually pulled from one star to another to form a massive, unusually hot star that appears younger than it is.

The research was part funded by the UK’s Science and Technology Facilities Council (STFC) and carried out by scientists at Southampton University and the McMaster University in Canada.

Blue stragglers are found throughout the Universe in globular clusters – collections of about 100, 000 stars, tightly bound by gravity.

According to conventional theories, the massive blue stragglers found in these clusters should have died long ago because all stars in a cluster are born at the same time and should therefore be at a similar phase.

These massive rogue stars, however, appear to be much younger than the other stars and are found in virtually every observed cluster.

“The origin of blue stragglers has been a long-standing mystery. The only thing that was clear is that at least two stars must be involved in the creation of every single blue straggler, because isolated stars this massive simply should not exist in these clusters,” said Dr Christian Knigge from Southampton University, who led the study.

“We’ve known of these stellar anomalies for 55 years now. Over time, two main theories have emerged: that blue stragglers were created through collisions with other stars; or that one star in a binary system was ‘reborn’ by pulling matter off its companion,” said Professor Alison Sills from the McMaster University.

The researchers looked at blue stragglers in 56 globular clusters.

They found that the total number of blue stragglers in a given cluster did not correlate with predicted collision rate – dispelling the theory that blue stragglers are created through collisions with other stars.

They did, however, discover a connection between the total mass contained in the core of the globular cluster and the number of blue stragglers observed within in.

Since more massive cores also contain more binary stars, they were able to infer a relationship between blue stragglers and binaries in globular clusters.

They also showed that this conclusion is supported by preliminary observations that directly measured the abundance of binary stars in cluster cores.

All of this points to “stellar cannibalism” as the primary mechanism for blue straggler formation.

According to Dr Knigge, “This is the strongest and most direct evidence to date that most blue stragglers, even those found in the cluster cores, are the offspring of two binary stars.” (ANI)