Skupina Honicích psů II

NGC 4288 GALEX WikiSky.jpg
NGC 4288 by GALEX

Messier 106 visible and infrared composite.jpg
A spiral galaxy with a secret

The NASA/ESA Hubble Space Telescope – with a little help from an amateur astronomer – has produced one of the best views yet of nearby spiral galaxy Messier 106. Located a little over 20 million light-years away, practically a neighbour by cosmic standards, Messier 106 is one of the brightest and nearest spiral galaxies to our own.

Despite its appearance, which looks much like countless other galaxies, Messier 106 hides a number of secrets. Thanks to this image, which combines data from Hubble with observations by amateur astronomers Robert Gendler and Jay GaBany, they are revealed as never before.

At its heart, as in most spiral galaxies, is a supermassive black hole, but this one is particularly active. Unlike the black hole at the centre of the Milky Way, which pulls in wisps of gas only occasionally, Messier 106’s black hole is actively gobbling up material. As the gas spirals towards the black hole, it heats up and emits powerful radiation. Part of the emission from the centre of Messier 106 is produced by a process that is somewhat similar to that in a laser - although here the process produces bright microwave radiation.^[1]

As well as this microwave emission from Messier 106’s heart, the galaxy has another startling feature - instead of two spiral arms, it appears to have four. Although the second pair of arms can be seen in visible light images as ghostly wisps of gas, as in this image, they are even more prominent in observations made outside of the visible spectrum, such as those using X-ray or radio waves.

Unlike the normal arms, these two extra arms are made up of hot gas rather than stars, and their origin remained unexplained until recently. Astronomers think that these, like the microwave emission from the galactic centre, are caused by the black hole at Messier 106’s heart, and so are a totally different phenomenon from the galaxy’s normal, star-filled arms.

The extra arms appear to be an indirect result of jets of material produced by the violent churning of matter around the black hole. As these jets travel through the galactic matter they disrupt and heat up the surrounding gas, which in turn excites the denser gas in the galactic plane and causes it to glow brightly. This denser gas closer to the centre of the galaxy is tightly-bound, and so the arms appear to be straight. However, the looser disc gas further out is blown above or below the disc in the opposite direction from the jet, so that the gas curves out of the disc — producing the arching red arms seen here.

Despite carrying his name, Messier 106 was neither discovered nor catalogued by the renowned 18th century astronomer Charles Messier. Discovered by his assistant, Pierre Méchain, the galaxy was never added to the catalogue in his lifetime. Along with six other objects discovered but not logged by the pair, Messier 106 was posthumously added to the Messier catalogue in the 20th century.

Amateur astronomer Robert Gendler retrieved archival Hubble images of M 106 to assemble a mosaic of the centre of the galaxy. He then used his own and fellow astrophotographer Jay GaBany’s observations of M 106 to combine with the Hubble data in areas where there was less coverage, and finally, to fill in the holes and gaps where no Hubble data existed.

The centre of the galaxy is composed almost entirely of Hubble data taken by the Advanced Camera for Surveys, Wide Field Camera 3, and Wide Field and Planetary Camera 2 detectors. The outer spiral arms are predominantly HST data colourised with ground-based data taken by Gendler’s and GaBany’s 12.5-inch and 20-inch telescopes, located at very dark remote sites in New Mexico, USA.

Gendler was a prizewinner in the recent Hubble’s Hidden Treasures image processing competition. Another prizewinner, André van der Hoeven, entered a different version of Messier 106, combining Hubble and NOAO data.

About the Object:

Name:	M 106
Type:	• Local Universe : Galaxy : Type : Spiral
	• Galaxies Images/Videos
Distance: 20 million light years

Colours & filters:

Band	Wavelength	Telescope
Infrared I	814 nm	Hubble Space Telescope ACS
Infrared I	814 nm	Hubble Space Telescope WFC3
Optical H-alpha	656 nm	Hubble Space Telescope WFPC2
Optical V	555 nm	Hubble Space Telescope ACS
Optical V	606 nm	Hubble Space Telescope ACS
Optical V	555 nm	Hubble Space Telescope WFC3
Optical B	435 nm	Hubble Space Telescope ACS

Footnotes

NGC4490 Galaxy from the Mount Lemmon SkyCenter Schulman Telescope courtesy Adam Block.jpg
Autor: Adam Block/Mount Lemmon SkyCenter/University of Arizona, Licence: CC BY-SA 3.0 us
Deep exposure of NGC 4490 using the 0.8m Schulman Telescope at the Mount Lemmon SkyCenter

• Optics 32-inch Schulman Telescope (RC Optical Systems), Acquired remotely
• Camera SBIG STX 16803 CCD Camera
• Filters AstroDon Gen II
• Dates March - April 2013
• Location Mount Lemmon SkyCenter
• Exposure LRGB = 7:2:2:2 hours
• Acquisition ACP Observatory Control Software (DC-3 Dreams),TheSky (Software Bisque), Maxim DL/CCD (Cyanogen), FlatMan XL (Alnitak)
• Processing CCDStack (CCDWare), Photoshop CS5 (Adobe), PixInsight
• Guest Astronomers Participants of the May 2013 CCD Image Processing Workshop

NGC 4707 GALEX WikiSky.jpg
NGC 4707 galaxy by GALEX

NGC 4096 GALEX WikiSky.jpg
NGC 4096 by GALEX

Canes II group.gif
Autor: Atlas of the Universe, Licence: CC BY-SA 3.0
Gruppo Canes II

NGC 4242 hst 06232 R814GB450 .png
Autor: Own work, Licence: CC BY-SA 3.0
Color rendering is done by by Aladin-software (2000A&AS..143...33B.)

NGC 4144 HST 9765 R814GB606.png
Autor: Own work, Licence: CC BY-SA 3.0
Color rendering is done by by Aladin-software (2000A&AS..143...33B.)