Frantic activity revealed in dusty stellar factories
Astronomers from the Instituto de Astrofísica de Canarias (Spain) used NACO, a sharp-eyed adaptive optics instrument on ESO's Very Large Telescope (VLT), to study the fine detail in NGC 253, one of the brightest and dustiest spiral galaxies in the sky. Adaptive Optics (AO) corrects for the blurring effect introduced by the Earth's atmosphere. This turbulence causes the stars to twinkle in a way that delights poets, but frustrates astronomers, since it smears out the images. With AO in action the telescope can produce images that are as sharp as is theoretically possible, as if the telescope were in space. NACO revealed features in the galaxy that were only 11 light-years across. "Our observations provide us with so much spatially resolved detail that we can, for the first time, compare them with the finest radio maps for this galaxy — maps that have existed for more than a decade," says Juan Antonio Fernández-Ontiveros, the lead author of the paper reporting the results [1].
Astronomers identified 37 distinct bright regions, a threefold increase on previous results, packed into a tiny region at the core of the galaxy, comprising just one percent of the galaxy's total size. The astronomers combined their NACO images with data from another VLT instrument, VISIR, as well as with images from the NASA/ESA Hubble Space Telescope and radio observations made by the Very Large Array and the Very Large Baseline Interferometer. Combining these observations, taken in different wavelength regimes, provided a clue to the nature of these regions.
"We now think that these are probably very active nurseries that contain many stars bursting from their dusty cocoons," says Jose Antonio Acosta-Pulido, a member of the team. NGC 253 is known as a starburst galaxy, after its very intense star formation activity. Each bright region could contain as many as one hundred thousand young, massive stars.
This comprehensive set of data also leads astronomers to conclude that the centre of NGC 253 hosts a scaled-up version of Sagittarius A*, the bright radio source that lies at the core of the Milky Way and which we know harbours a massive black hole (see ESO 46/08). "We have thus discovered what could be a twin of our Galaxy's Centre," says co-author Almudena Prieto.
Source: ESO
Related
- Astronomers discover link between supermassive black holes and galaxy formationMon, 2 Feb 2009, 17:07:42 EST
- University of Hawaii at Manoa astronomer finds giant galaxyThu, 3 Sep 2009, 9:39:51 EDT
- Stellar family in crowded, violent neighborhood proves to be surprisingly normalThu, 4 Jun 2009, 9:50:33 EDT
- NGC 4945: The Milky Way's not-so-distant cousinWed, 2 Sep 2009, 9:39:34 EDT
- Watching a 'new star' make the Universe dustyThu, 24 Jul 2008, 13:29:53 EDT
Other sources
- Frantic Activity Revealed In Dusty Stellar Factoriesfrom Science DailyMon, 19 Jan 2009, 15:21:18 EST
- Found: Stellar Nurseries In NGC 253 And A Black Hole 'Twin' Of Our Milky Way's Sagittarius A*from Scientific BloggingMon, 19 Jan 2009, 14:49:20 EST
- Frantic activity revealed in dusty stellar factoriesfrom PhysorgMon, 19 Jan 2009, 12:28:04 EST
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