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Astronomie - Herschel enthüllt Serpens Kern, das Herz einer riesigen molekularen Wolke

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  • Title Herschel reveals filaments in the Serpens Core
  • Released 18/01/2016 12:40 pm
  • Copyright ESA/Herschel/PACS/SPIRE/V. Roccatagliata (U. München, Germany)
  • Description

    The interstellar medium fills the ‘empty’ space between the stars in our galaxy. It is a mix of molecular clouds, cold and warm gases, regions of electrically charged hydrogen, and more.

    Molecular clouds are the densest part of the interstellar medium, holding most of its mass in the form of hydrogen gas. ESA’s Herschel space observatory has revealed that many are built around filaments, with dense threads snaking throughout each cloud. These filaments potentially transport material, and, when massive enough, are known to form new stars.

    This Herschel image shows the Serpens Core, the heart of a giant molecular cloud. The Core is the bright clump towards the upper right, with a more diffuse secondary cluster, named Ser G3-G6, shown at the bottom right. Also visible as a faint yellow glow towards the upper left of the frame is a region known as LDN 583 that shines brightly in the far-infrared.

    Giant molecular clouds contain up to 10 million times the mass of the Sun, and can stretch for hundreds of light-years. Compared to the rest of space they are dense, holding up to a thousand atoms per cubic centimetre – and even more in star-forming regions. However, these properties are relative: even at their densest, these clouds are more than 10 times emptier than the best laboratory vacuums we can produce on Earth.

    These giant clouds are complex formations, most often made up of filaments mixed with clumpy and irregular folds, sheets and bubble-like structures. A typical spiral galaxy like the Milky Way can contain thousands of them, accompanied by many of their smaller relatives.

    Serpens is an ideal target for scientists wanting to know more about giant molecular clouds, because it lies just 1400 light-years from us. Scientists compared Herschel’s observations of this cloud to a state-of-the-art simulation to find out more about the cloud’s properties, and to test the accuracy of their model.

    They discovered a radial network of filaments stretching throughout the Serpens Core, filaments that are predicted to break and fragment to form the cores of new stars. These filaments resemble the spokes of a wheel, with the Core forming the hub.

    This three-colour image is made from observations with Herschel’s PACS camera (blue and green) and SPIRE camera (red). The size of the region shown is 1.7x1.9º on the sky, where 1º corresponds to about 25 light-years.

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The intricate jumble depicted in this image from ESA’s Herschel space observatory shows the distribution of gas and dust in the Taurus Molecular Cloud, a giant stellar nursery about 450 light-years away in the constellation Taurus, the Bull.
Launched in 2009, Herschel studied the sky at far-infrared wavelengths for almost four years, detecting the glow of cosmic dust in the interstellar medium that pervades our Galaxy, the Milky Way. Dust is a minor but crucial ingredient in this diffuse mixture that provides the raw material for stars to form.
One of the observatory’s most striking discoveries was the detection of ubiquitous filaments – elongated and thin structures of gas and dust weaving their way across the Galaxy. Interstellar filaments were already known before Herschel, but the new data revealed them almost everywhere in the Milky Way and highlighted their role as preferred hubs for stellar birth.
Astronomers now believe that filaments precede the onset of most star formation, funnelling interstellar gas and dust into increasingly denser concentrations. Gravity later causes the densest filaments to contract and fragment, eventually leading to the formation of stars.
This image shows a tangle of filaments emerging from the cloud material, which are dotted with a few compact, bright cores: the seeds of future stars. The view also reveals a network of smaller threads, perpendicular to the most prominent filament.
This pattern is suggestive of accretion flows, indicating that the material along filaments is not at all static and that the most massive among them might be drawing matter from their surroundings. Some numerical simulations of star formation in molecular clouds also predict a similar arrangement of interstellar material, with gas and dust streaming towards the densest filaments along routes that are shaped by the local magnetic field.
This three-colour image combines Herschel bands at 160 microns (blue), 250 microns (green) and 500 microns (red), and spans about 5º on the long side. The data were acquired with Herschel as part of the Gould Belt survey Key Programme in 2010 and 2012, and a study of the filamentary structure is presented in a paper by P. Palmeirim et al. 2013. The image was first published on ESA’s Science and Technology website in May 2015.
Quelle: ESA
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