Wednesday, September 30, 2015

Southern African Large Telescope reveals too large a black hole

The Southern African Large Telescope (SALT), Africa’s most powerful eye on the sky, has been used to discover a supermassive black hole in the centre of a modest galaxy, SAGE0536AGN. All but the smallest galaxies are thought to harbour a black hole, but in this case the black hole was found to be thirty times more massive than what one would have expected for this size galaxy. It leaves scientists scratching their heads in pursuit of an explanation.

The presence of a black hole was suspected when the infrared emission from its dusty environs was discovered in 2009 using NASA’s Spitzer Space Telescope. Now, scientists from the United Kingdom SALT Consortium, Jacco van Loon from Keele University and Anne Sansom from the University of Central Lancashire used the SALT to take a spectrum of the galaxy. The spectrum showed emission at particular wavelengths related to hydrogen gas, but shifted to redder wavelengths than on Earth due to the large recession velocity of the galaxy, placing it at a distance from which light took 1.86 billion years to reach us. This already indicated that the central engine of the galaxy must be very luminous. The spread in wavelength of the hydrogen emission betrayed gas moving very rapidly in the strong gravitational field of the black hole, and from this the mass of the black hole was determined to be 350 million times that of the Sun. For comparison, this is a hundred times more massive than the black hole that lives in the centre of our own Milky Way. However, when they also measured the mass of the galaxy itself, from the absorption of light by heavier atoms, they were surprised to find the galaxy’s mass to be a mere 25 billion times that of the Sun, less than that of the Milky Way!

Says Jacco van Loon: “For a long time, scientists have been trying to explain the good observed relationship between the mass of the black hole and the mass of the galaxy host. Now they will need to start explaining how some systems can deviate so much from this relationship.”
Because the galaxy was only found by accident in the distant background of a survey meant to study a very nearby dwarf galaxy, surveys aimed at finding extragalactic supermassive black holes may have missed more systems like SAGE0536AGN. SALT may thus have opened a new window, and a new view of how galaxies and their central engines have grown over time.

An image of the galaxy SAGE0536AGN, from the Vista Magellanic Clouds survey. The galaxy is the elliptical object in the centre of the image. (Credit: Vista Magellanic Clouds survey)

Night Log 2015-09-29

SA: Brent
SO: Veronica
Others: Chris, Eben, Eric, Mexican delegation

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Extensive heavy clouds tonight. No observations possible.

Tuesday, September 29, 2015

Night Log 2015-09-28

SA: Brent
SO: Veronica
Others:

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A frustrating night with a lot of cloud. Managed to take data for:

2015-1-SCI-037 P2 HRS (x2) (Exploring the limits of HRS for measuring Exoplanet Radial Velocities)
2015-1-SCI-045 P3 RSS (x2) (Searching for binaries in unusual central stars of planetary nebulae)
2015-1-SCI-059 P4 RSS (x2) (Long term monitoring of the SMC LBV S18 and LMC sgB[e] star S134)

Monday, September 28, 2015

Night Log 2015-09-27

SA: Brent
SO: Veronica
Others: Lunar eclipse!!

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Too humid to observe tonight. The lunar eclipse was magnificent!

Sunday, September 27, 2015

Night Log 2015-09-26

SA: Brent
SO: Veronica
Others:

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Night lost to bad weather.

Saturday, September 26, 2015

Night Log 2015-09-25

SA: Brent
SO: Veronica
Others:

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Mostly clear, bright night with around 2 arcsec seeing. Clouds rolled over around 2:30 forcing us to close.

Data taken for:

2015-1-SCI-063 P0 RSS (SALT follow-up of type Ia supernovae to study their properties at targeted redshifts)
2015-1-SCI-028 P1 HRS (Looking for evidence of massive white dwarfs in symbiotic novae)
2015-1-SCI-037 P2 HRS (Exploring the limits of HRS for measuring Exoplanet Radial Velocities)
2015-1-SCI-011 P3 RSS (Searching the Milky Way for symbiotic stars)
2015-1-SCI-045 P3 RSS (Searching for binaries in unusual central stars of planetary nebulae)
2015-1-SCI-005 P3 RSS (Time variability of emerging BAL QSOs.)

Friday, September 25, 2015

Night Log 2015-09-24

SA: Brent
SO: Veronica
Others: evil brommers everywhere

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A rather busy bright clear night with mostly very good seeing. Some engineering data taken as well as data taken for:

2015-1-DDT-006 P1 RSS (DDT request)
2015-1-SCI-065 P1 RSS (x2) (FP Halpha kinematics of RESOLVE galaxies)
2015-1-SCI-013 P1 HRS (Evolved binaries in the Magellanic Clouds )
2015-1-SCI-028 P1 HRS (Looking for evidence of massive white dwarfs in symbiotic novae)
2015-1-SCI-037 P2 HRS (Exploring the limits of HRS for measuring Exoplanet Radial Velocities)
2015-1-SCI-017 P3 RSS (Observations of evolved massive stars revealed with Spitzer and WISE)