VLT finds a brilliant but solitary superstar

May 25, 2011
This view shows part of the very active star-forming region around the Tarantula Nebula in the Large Magellanic Cloud, a small neighbour of the Milky Way. At the exact centre lies the brilliant but isolated star VFTS 682 and to its lower right the very rich star cluster R 136. The origins of VFTS are unclear — was it ejected from R 136 or did it form on its own? The star appears yellow-red in this view, which includes both visible-light and infrared images from the Wide Field Imager at the 2.2-metre MPG/ESO telescope at La Silla and the 4.1-metre infrared VISTA telescope at Paranal, because of the effects of dust. Credit: ESO/M.-R. Cioni/VISTA Magellanic Cloud survey. Acknowledgment: Cambridge Astronomical Survey Unit

(PhysOrg.com) -- An extraordinarily bright isolated star has been found in a nearby galaxy -- the star is three million times brighter than the Sun. All previous similar "superstars" were found in star clusters, but this brilliant beacon shines in solitary splendour. The origin of this star is mysterious: did it form in isolation or was it ejected from a cluster? Either option challenges astronomers’ understanding of star formation.

An international team of astronomers has used ESO’s Very Large Telescope to carefully study the star VFTS 682 in the , a small neighbouring galaxy to the Milky Way. By analysing the star’s light, using the FLAMES instrument on the VLT, they have found that it is about 150 times the mass of the Sun. Stars like these have so far only been found in the crowded centres of star clusters, but VFTS 682 lies on its own.

“We were very surprised to find such a massive star on its own, and not in a rich star cluster,” notes Joachim Bestenlehner, the lead author of the new study and a student at Armagh Observatory in Northern Ireland. “Its origin is mysterious.”

This star was spotted earlier in a survey of the most brilliant stars in and around the Tarantula Nebula in the Large Magellanic Cloud. It lies in a stellar nursery: a huge region of gas, dust and young stars that is the most active star-forming region in the Local Group of galaxies. At first glance VFTS 682 was thought to be hot, young and bright, but unremarkable. But the new study using the VLT has found that much of the star’s energy is being absorbed and scattered by dust clouds before it gets to Earth — it is actually more luminous than previously thought and among the brightest stars known.

Red and infrared light emitted by the star can get through the dust, but the shorter-wavelength blue and green light is scattered more and lost. As a result the star appears reddish, although if the view were unobstructed it would shine a brilliant blue-white.

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This sequence starts with a view of the Milky Way and its two small neighbouring galaxies, the Magellanic Clouds. We zoom in towards the Large Magellanic Cloud and focus on the huge star formation region around the Tarantula Nebula. The final sequence shows a very detailed view, captured in both visible and infrared light, of the dense star cluster R 136 and the very brilliant, but strangely isolated, star VFTS 682. Credit: ESO/Digitized Sky Survey 2/R. Gendler/S. Brunier. Music: John Dyson (from the album Moonwind)

As well as being very bright, VFTS 682 is also very hot, with a surface temperature of about 50 000 degrees Celsius. Stars with these unusual properties may end their short lives not just as a supernova, as is normal for high-mass stars, but just possibly as an even more dramatic long-duration gamma-ray burst, the brightest explosions in the Universe.

Although VFTS 682 seems to now be alone it is not very far away from the very rich star cluster RMC 136 (often called just R 136), which contains several similar “superstars”.

“The new results show that VFTS 682 is a near identical twin of one of the brightest superstars at the heart of the R 136 star cluster,” adds Paco Najarro, another member of the team from CAB (INTA-CSIC, Spain).

Is it possible that VFTS 682 formed there and was ejected? Such “runaway stars” are known, but all are much smaller than VFTS 682 and it would be interesting to see how such a heavy star could be thrown from the cluster by gravitational interactions.

“It seems to be easier to form the biggest and brightest in rich ,” adds Jorick Vink, another member of the team. “And although it may be possible, it is harder to understand how these brilliant beacons could form on their own. This makes VFTS 682 a really fascinating object.”

Explore further: Image: Galactic wheel of life shines in infrared

More information: This research was presented in a paper, “The VLT-FLAMES Tarantula Survey III: A very massive star in apparent isolation from the massive cluster R136”, to appear in Astronomy & Astrophysics. arxiv.org/abs/1105.1775

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omatumr
1 / 5 (8) May 25, 2011
We were very surprised to find such a massive star on its own, and not in a rich star cluster, notes Joachim Bestenlehner, the lead author of the new study and a student at Armagh Observatory in Northern Ireland. Its origin is mysterious.


Congratulations!

You are on the right path to discovery.

Please avoid the disease that plagues modern science:

"To know that you do not know is best.
To pretend to know what you do not know is a disease."
Lao-tse (~500 BC)

With kind regards,
Oliver K. Manuel
that_guy
4 / 5 (4) May 25, 2011
So why have you not taken your neutron information to other scientists who know better in other areas than your own? Why do you think that you know best about everything Oliver?

Tseihta
5 / 5 (3) May 31, 2011
Is anyone else tired of scrolling though the endless nonsensical posts from Oliver K. Manuel? omatumr is SPAMMING this site with ramblings of PSEUDO-SCIENCE?

Hey Moderators... I thought this sort of behaviour is not permitted on this site?? Do us all a favour and follow your own rules and fix this.
omatumr
1 / 5 (5) May 31, 2011
1. As well as being very bright, VFTS 682 is also very hot, with a surface temperature of about 50 000 degrees Celsius. Stars with these unusual properties may end their short lives not just as a supernova, as is normal for high-mass stars, but just possibly as an even more dramatic long-duration gamma-ray burst, the brightest explosions in the Universe.

2. As well as being very bright, VFTS 682 is also very hot, with a surface temperature of about 50 000 degrees Celsius. Stars with these unusual properties may end their short lives not just as a supernova, as is normal for high-mass stars, but just possibly as an even more dramatic long-duration gamma-ray burst, the brightest explosions in the Universe.


These statement suggest that VFTS 682 may, like Sol, be the glowing waste products from a neutron star.

Glowing = Emitting photons

"Neutron Repulsion", The APEIRON Journal, in press, 19 pages (2011)

http://arxiv.org/...2.1499v1