NGC 371
 | |
| Aufnahme des VLTs | |
| AladinLite | |
| Sternbild | Tukan |
| Position Äquinoktium: J2000.0 | |
|---|---|
| Rektaszension | 01h 03m 25s [1] |
| Deklination | -72° 04′ 24″ [1] |
| Erscheinungsbild | |
| Winkelausdehnung | 7,5' [2] |
| Rötung (Farbexzess E(B-V)) | 0,037 [3] |
| Physikalische Daten | |
| Zugehörigkeit | KMW [2] |
| Geschichte | |
| Entdeckt von | James Dunlop |
| Entdeckungszeit | 1. August 1826 |
| Katalogbezeichnungen | |
| NGC 371 • Mel 5 • Dun 31 • ESO 51-SC14 • GC 198 • h 2376 • Lindsay 71 • Kron 48 • Henize 1997 | |
NGC 371 ist ein offener Sternhaufen umgeben von dem Emissionsnebel (HII-Region)[4] N76A in der etwa 200.000 Lichtjahre entfernten Kleinen Magellanschen Wolke. NGC 371 befindet sich im Sternbild Tukan.
NGC 371 wurde am 1. August 1826 von dem schottischen Astronomen James Dunlop entdeckt.[5] Die Sterne des offenen Sternhaufens entstehen aus dem leuchtenden Wasserstoff-Gas der HII-Region.[4] Dieser Sternhaufen hat ungewöhnlich viele Veränderliche Sterne u. a. langsam pulsierende B Sterne (LPS).
Weblinks
- Ralph-Mirko Richter: Der offene Sternhaufen NGC 371, 4. April 2011
- ESO: Das rosarote Glimmen der Sterngeburt +Foto, Karte und Animation – 30. März 2011
Einzelnachweise
- ↑ SIMBAD Database
- ↑ a b SEDS: NGC 371
- ↑ NASA/IPAC EXTRAGALACTIC DATABASE
- ↑ a b ESO (2011) The Rose-red Glow of Star Formation, 30 March 2011 (abgerufen am 5. April 2011)
- ↑ Seligman
Auf dieser Seite verwendete Medien
Autor/Urheber: ESO/Manu Mejias, Lizenz: CC BY 4.0
This picture of the star cluster and surrounding nebula NGC 371 was taken using the FORS1 instrument on ESO’s Very Large Telescope, at the Paranal Observatory in Chile. NGC 371 lies in the Small Magellanic Cloud, one of the closest galaxies to the Milky Way.
The vivid red cloud in this new image from ESO’s Very Large Telescope is a region of glowing hydrogen surrounding the star cluster NGC 371. This stellar nursery lies in our neighbouring galaxy, the Small Magellanic Cloud.
The object dominating this image may resemble a pool of spilled blood, but rather than being associated with death, such regions of ionised hydrogen — known as HII regions — are sites of creation with high rates of recent star birth. NGC 371 is an example of this; it is an open cluster surrounded by a nebula. The stars in open clusters all originate from the same diffuse HII region, and over time the majority of the hydrogen is used up by star formation, leaving behind a shell of hydrogen such as the one in this image, along with a cluster of hot young stars.
The host galaxy to NGC 371, the Small Magellanic Cloud, is a dwarf galaxy a mere 200 000 light-years away, which makes it one of the closest galaxies to the Milky Way. In addition, the Small Magellanic Cloud contains stars at all stages of their evolution; from the highly luminous young stars found in NGC 371 to supernova remnants of dead stars. These energetic youngsters emit copious amounts of ultraviolet radiation causing surrounding gas, such as leftover hydrogen from their parent nebula, to light up with a colourful glow that extends for hundreds of light-years in every direction. The phenomenon is depicted beautifully in this image, taken using the FORS1 instrument on ESO’s Very Large Telescope (VLT).
Open clusters are by no means rare; there are numerous fine examples in our own Milky Way. However, NGC 371 is of particular interest due to the unexpectedly large number of variable stars it contains. These are stars that change in brightness over time. A particularly interesting type of variable star, known as slowly pulsating B stars, can also be used to study the interior of stars through asteroseismology [1], and several of these have been confirmed in this cluster. Variable stars play a pivotal role in astronomy: some types are invaluable for determining distances to far-off galaxies and the age of the Universe.
The data for this image were selected from the ESO archive by Manu Mejias as part of the Hidden Treasures competition [2]. Three of Manu’s images made the top twenty; his picture of NGC 371 was ranked sixth in the competition. Notes
[1] Asteroseismology is the study of the internal structure of pulsating stars by looking at the different frequencies at which they oscillate. This is a similar approach to the study of the structure of the Earth by looking at earthquakes and how their oscillations travel through the interior of the planet.
[2] ESO’s Hidden Treasures 2010 competition gave amateur astronomers the opportunity to search through ESO’s vast archives of astronomical data, hoping to find a well-hidden gem that needed polishing by the entrants. Participants submitted nearly 100 entries and ten skilled people were awarded some extremely attractive prizes, including an all expenses paid trip for the overall winner to ESO’s Very Large Telescope (VLT) on Cerro Paranal, in Chile, the world’s most advanced optical telescope. The ten winners submitted a total of 20 images that were ranked as the highest entries in the competition out of the near 100 images.
Colours & filters Band Telescope Optical HeII Very Large Telescope FORS1 Optical HeI Very Large Telescope FORS1 Optical H-alpha Very Large Telescope FORS1.