phone Help-contact

Science Source Feb 2010

EN_90286391_0334
Science Source Feb 2010
  • 30,00 EUR

    Making print for private purpose, storage in computer memory, no distribution rights.

  • 40,00 EUR

    Strictly for editorial, single use on a personal (nonprofit) web site, Internet portal, social media (Facebook, Instagram etc.), blog for 1 year. Not for resale. Maximum picture size 2000px.

  • 75,00 EUR

    Strictly for editorial, single use on a commercial web site, Internet portal, social media (Facebook, Instagram etc.), blog for 1 year. Not for resale. Maximum picture size 2000px.

  • 90,00 EUR

    Strictly for editorial, single use, inside of newspaper, magazine, book (including digital version), one edition, one single country. Not for resale.

Gross prices
Contact us to calculate price for another use. Prices only for online sales.
This Chandra X-ray Observatory image shows Westerlund 2, a young star cluster with an estimated age of about one or two million years. Until recently little was known about this cluster because it is heavily obscured by dust and gas. However, using infrared and X-ray observations to overcome this obscuration, Westerlund 2 has become regarded as one of the most interesting star clusters in the Milky Way galaxy. It contains some of the hottest, brightest and most massive stars known. This image shows low energy X-rays in red, intermediate energy X-rays in green and high energy X-rays in blue. The image shows a very high density of massive stars that are bright in X-rays, plus diffuse X-ray emission. An incredibly massive double star system called WR20a is visible as the bright yellow point just below and to the right of the cluster's center. This system contains stars with masses of 82 and 83 times that of the Sun. The dense streams of matter steadily ejected by these two massive stars, called stellar winds, collide with each other and produce copious amounts of X-ray emission. This collision is seen at different angles as the stars orbit around each other every 3.7 days. Several other bright X-ray sources may also show evidence for collisions between winds in massive binary systems.
2010-02-13
EAST NEWS
Science Source
NASA
bj4953
0,46MB
36cm x 36cm by 300dpi
2, 82, 83, ABOUT, AGE, ALSO, AMOUNTS, AN, AND, ANGLES, ARE, AROUND, AS, ASTRONOMICAL, ASTRONOMY, ASTROPHOTOGRAPHY, AT, BECAUSE, BECOME, BELOW, BETWEEN, BINARY, BLUE, BRIGHT, BRIGHTEST, BY, CALLED, CENTER, CHANDRA, CLUSTER, CLUSTERS, COLLIDE, COLLISION, COLLISIONS, CONTAINS, COPIOUS, DAYS, DENSE, DENSITY, DIFFERENT, DIFFUSE, DOUBLE, DOUBLE-STAR, DUST, EACH, EJECTED, EMISSION, ENERGY, ESTIMATED, EVERY, EVIDENCE, FOR, GALAXY, GAS, GREEN, HAS, HEAVILY, HIGH, HOTTEST, HOWEVER, IMAGE, IN, INCREDIBLY, INFRARED, INTERESTING, INTERMEDIATE, IS, IT, JUST, KNOWN, LITTLE, LOW, MASSES, MASSIVE, MATTER, MAY, MILKY, MILLION, MOST, NASA, OBSCURATION, OBSCURED, OBSERVATIONS, OBSERVATORY, OF, ONE, OR, ORBIT, OTHER, OVERCOME, PHOTOGRAPHY, PLUS, POINT, PRODUCE, RECENTLY, RED, REGARDED, RIGHT, SEEN, SEVERAL, SHOW, SHOWS, SOME, SOURCES, STAR, STARS, START, STEADILY, STELLAR, STREAMS, SUN, SYSTEM, SYSTEMS, THAT, THE, THESE, THIS, TIMES, TO, TWO, UNTIL, USING, VERY, VISIBLE, WAS, WAY, WESTERLUND, WIND, WINDS, WITH, WR20A, X-RAY, X-RAYS, YEARS, YELLOW, YOUNG,