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    Theta1 Orionis C Looks Like A 'Santa Claus' In Space
    By News Staff | November 30th 2007 10:09 AM | Print | E-mail | Track Comments
    Right in time for the festive season, ESA's XMM-Newton X-ray observatory has discovered a huge cloud of high-temperature gas resting in a spectacular nearby star-forming region, shaped somewhat like the silhouette of Santa Claus.

    An early present for astronomers, the cloud suggests that hot gas from many star-forming regions leaks into the interstellar medium.

    The Orion nebula is the nearest dense star-forming region to Earth that contains stars much more massive than the Sun. XMM-Newton’s newly-discovered gas cloud is composed of winds blowing from these high-mass stars that are heated to millions of degrees as they slam into the surrounding gas.

    CLICK IMAGE ABOVE FOR FULL SIZE.
    The images show the Orion nebula with its hot gas cloud. The left panel is an image obtained with XMM-Newton data from its European Photon Imaging Camera in X-rays. The right panel shows XMM-Newton data, compared to Spitzer observations of the same region. The Spitzer image is a composite image of data obtained in the infrared. The Orion nebula is the nearest dense star-forming region to Earth that contains stars much more massive than the Sun. XMM-Newton’s newly-discovered gas cloud is composed of winds blowing from these high-mass stars that are heated to millions of degrees as they slam into the surrounding gas. Credit: Panel A: XMM-Newton EPIC (Guedel et al.), Panel B: AAAS/Science (ESA XMM-Newton and NASA Spitzer data)



    “There is one star in particular that dominates the nebula,” says Manuel Güdel, Paul Scherrer Institut, Switzerland, who led the team that discovered the gas. The star in question is theta1 Orionis C, a giant star around 40 times mass of the Sun, with a surface temperature of 40,000°C. Güdel and his colleagues think that the violent collision between the wind from this star and the surrounding dense gas is largely responsible for the newly-discovered hot gas cloud.

    The high-temperature gas fills a region of the nebula that appears to be a huge cavity in optical and infrared images. The new observations, taken with XMM-Newton’s European Photon Imaging Camera (EPIC) camera, suggest that astronomers are seeing only a particular portion of the gas. The X-rays from this portion escape absorption by patches of cold gas covering much of the front of the Orion nebula.

    CLICK IMAGE ABOVE FOR FULL SIZE.
    This is a multi-wavelength image of the Orion nebula. Panel A and B are Spitzer images overlaid with XMM-Newton data. Panel C is an optical image obtained with the UK Schmidt telescope overlaid with XMM-Newton data. Panel D contains the same UK Schmidt telescope image with overlays of radio data from the Very Large Array. Credits: Panel A: AAAS/Science (ESA XMM-Newton and NASA Spitzer data) B: NASA/ Spitzer, C: © Anglo-Australian Observatory/David Malin Images, D: © Anglo-Australian Observatory/David Malin Images, VLA



    The surrounding pattern of absorbing clouds gives the detected gas its Santa Claus shape, with his prominent hat outlined by the northern gas bubble. In its entirety, the hot gas probably fills the whole nebula.

    The team discovered it whilst conducting a survey of the young stars in the region. In the background of many of those images was a faint glow of X-rays. “The diffuse signal came up time and time again. Finally, we realized that it was something real,” says Güdel.

    The presence of the hot gas in a fairly common nebula like Orion is surprising. Although theory has predicted such hot gas clouds, previous observations suggested that a large number of massive stars shedding winds, or supernova explosions are required. These are found in some regions of vigorous high-mass star formation, which are scattered only rarely throughout the galaxy. The new observations show that much smaller collections of high mass stars can produce hot gas as well.

    CLICK IMAGE ABOVE FOR FULL SIZE.
    The Orion nebula, some features are labelled. Credits: © Anglo-Australian Observatory/David Malin Images



    There are many star-forming regions similar to the Orion nebula throughout the galaxy, so there should be a network of channels and bubbles being filled up by the hot gas leaking from these various regions. “This is another possible way to enrich the interstellar medium. You don’t have to wait for a sudden supernova to explode. You can do it with just one or two massive stars over millions of years,” says Güdel.

    The team now plans to obtain new observations to determine how the gas flows out of the Orion nebula. In particular, they want to see whether it connects with a giant bubble created by supernova explosions from previous generations of massive stars.