Showing posts with label Hungry. Show all posts
Showing posts with label Hungry. Show all posts

Wednesday, October 8, 2014

ICRAR: Hungry black hole consumes material faster than thought possible

A rendering of what Black Hole P13 would look like close up. 

Credit: by Tom Russell (ICRAR) using software created by Rob Hynes (Louisiana State University).

Astronomers have discovered a black hole that is consuming gas from a nearby star 10 times faster than previously thought possible.

The black hole, known as P13, lies on the outskirts of the galaxy NGC7793 about 12 million light years from Earth and is ingesting a weight equivalent to 100 billion billion hot dogs every minute.

The discovery was published today in the journal Nature.

International Centre for Radio Astronomy Research (ICRAR) astronomer Dr Roberto Soria, who is based at ICRAR's Curtin University node, said that as gas falls towards a black hole it gets very hot and bright.

He said scientists first noticed P13 because it was a lot more luminous than other black holes, but it was initially assumed that it was simply bigger.

"It was generally believed the maximum speed at which a black hole could swallow gas and produce light was tightly determined by its size," Dr Soria said.

"So it made sense to assume that P13 was bigger than the ordinary, less bright black holes we see in our own galaxy, the Milky Way."

When Dr Soria and his colleagues from the University of Strasbourg measured the mass of P13 they found it was actually on the small side, despite being at least a million times brighter than the Sun.

It was only then that they realised just how much material it was consuming.

"There's not really a strict limit like we thought, black holes can actually consume more gas and produce more light," Dr Soria said.

Dr Soria said P13 rotates around a supergiant 'donor' star 20 times heavier than our own Sun.

He said the scientists saw that one side of the donor star was always brighter than the other because it was illuminated by X-rays coming from near the black hole, so the star appeared brighter or fainter as it went around P13.

Primary Image: This is a combined optical /X-ray image of NGC 7793

Inset image: This is a rendering of what P13 would look like close up. 

Credit: X-ray (NASA /CXC /Univ of Strasbourg /M. Pakull et al); Optical (ESO /VLT /Univ of Strasbourg /M. Pakull et al); H-alpha (NOAO /AURA /NSF /CTIO 1.5m). 

Insert Image: created by Tom Russell (ICRAR) using software created by Rob Hynes (Louisiana State University).

"This allowed us to measure the time it takes for the black hole and the donor star to rotate around each other, which is 64 days, and to model the velocity of the two objects and the shape of the orbit," Dr Soria said.

"From this, we worked out that the black hole must be less than 15 times the mass of our Sun."

Dr Soria said P13 is a member of a select group of black holes known as ultraluminous X-ray sources.

"These are the champions of competitive gas eating in the Universe, capable of swallowing their donor star in less than a million years, which is a very short time on cosmic scales," he said.

More information: 'A mass of less than 15 solar masses for the black hole in an ultraluminous X-ray source' was published in Nature, 9 October 2014. C. Motch, M. W. Pakull, R. Soria, F. Grise, G. Pietrzynski. DOI: 10.1038/nature13730

Sunday, May 4, 2014

ESA Hubble View: NGC 4303 A Hungry Starburst Galaxy

This new ESA Hubble picture is the sharpest ever image of the core of spiral galaxy Messier 61. 

Taken using the High Resolution Channel of Hubble's Advanced Camera for Surveys (ACS), the central part of the galaxy is shown in striking detail.

Credit: European Space Agency

Also known as NGC 4303, this galaxy is roughly 100,000 light-years across, comparable in size to our galaxy, the Milky Way.

Both Messier 61 and our home galaxy belong to a group of galaxies known as the Virgo Supercluster in the constellation of Virgo (The Virgin), a group of galaxy clusters containing up to 2,000 spiral and elliptical galaxies in total.

Messier 61 is a type of galaxy known as a starburst galaxy, one that experiences an incredibly high rate of star formation, hungrily using up their reservoir of gas in a very short period of time (in astronomical terms).

But this is not the only activity going on within the galaxy; deep at its heart there is thought to be a supermassive black hole that is violently spewing out radiation.

Despite its inclusion in the Messier Catalogue, Messier 61 was actually discovered by Italian astronomer Barnabus Oriani in 1779.

Charles Messier also noticed this galaxy on the very same day as Oriani, but mistook it for a passing comet, the comet of 1779.