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Showing posts with label SOAR Telescope. Show all posts
Showing posts with label SOAR Telescope. Show all posts

Wednesday, February 26, 2014

NGC 5044


This image shows a composite view of the giant elliptical galaxy NGC 5044.

The stellar component, as observed at optical wavelengths, is shown in white at the center of the image. The other stars scattered around the image are foreground stars from our own Galaxy.

The galaxy is embedded in a hot atmosphere of ionized hydrogen gas, which is shown in blue. With temperatures up to tens of millions of K, the hot gas shines brightly in X-rays and was observed using NASA's Chandra X-ray Observatory.

Observations show that some of the hot gas cools down and flows towards the center of the galaxy. There, the cold gas may condense and form stars, unless it is reheated or expelled from the galaxy by other agents.

The filamentary network shown in red is warm hydrogen gas, as observed in the H-alpha emission line at a rest wavelength of 656.28 nm with the Southern Observatory for Astrophysical Research (SOAR) telescope in Chile.

When observed in radio wavelengths, this galaxy appears only as the weak source shown in violet at the center of the image, which belies the moderately active black hole sitting at the center of the galaxy. The radio observations were performed with NRAO's Very Large Array (VLA).

A team of astronomers has observed NGC 5044 and other nearby giant elliptical galaxies using ESA's Herschel Space Observatory, to try to figure out why galaxies of this type do not form stars. Spectroscopic observations obtained with Herschel showed that, contrary to previous belief, NGC 5044 contains plenty of cold gas – the raw material to form stars. The same holds true for most of the giant elliptical galaxies that the team observed.

A multi-wavelength study suggests that, while hot gas cools down in these galaxies, stars do not form because of feedback from the central supermassive black hole, which stirs up the gas preventing it from turning into stars.

Image credit: Digitized Sky Survey/NASA Chandra/Southern Observatory for Astrophysical Research/Very Large Array (Robert Dunn et al. 2010)

Note: For more information, see Bullying Black Holes Force Galaxies to Stay Red and Dead.

Thursday, January 12, 2012

Galaxy Cluster ACT-CL J0102−4915 - "El Gordo"


This picture of the galaxy cluster ACT-CL J0102−4915 combines images taken with ESO’s Very Large Telescope with images from the SOAR Telescope and X-ray observations from NASA’s Chandra X-ray Observatory. The X-ray image shows the hot gas in the cluster and is shown in blue. This newly discovered galaxy cluster has been nicknamed El Gordo — the "big" or "fat one" in Spanish. It consists of two separate galaxy subclusters colliding at several million kilometers per hour, and is so far away that its light has traveled for seven billion years to reach the Earth.

Photo credit: ESO/SOAR/NASA

Note: For more information, see El Gordo — A “Fat” Distant Galaxy Cluster. Also, see El Gordo (ACT-CL J0102-4915):
NASA's Chandra Finds Largest Galaxy Cluster in Early Universe
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