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Chandra Sheds New Light On McNeil's Nebula

Date:
July 29, 2004
Source:
NASA/Marshall Space Flight Center
Summary:
The X-ray/optical comparison of the region surrounding McNeil's Nebula shows that the position of a source detected by NASA's Chandra X-ray Observatory is coincident with that of a bright infrared and optical source at the apex of the nebula.

Chandra X-ray Observatory Image of X-ray outburst from young star in McNeil's Nebula.
Credit: Image courtesy of NASA/Marshall Space Flight Center

The X-ray/optical comparison of the region surrounding McNeil's Nebula shows that the position of a source detected by NASA's Chandra X-ray Observatory is coincident with that of a bright infrared and optical source at the apex of the nebula. Source 3 is thought to be a very young star and is illuminating the fan-shaped cloud of gas, or nebula. The others sources in the field, labeled 1, 2, and 4, are other young, X-ray emitting stars in the region.

The small nebula, which lies in the constellation Orion about 1300 light years from Earth, was discovered with a 3-inch telescope by amateur astronomer Jay McNeil in January 2004. A young star buried deep in a cloud had brightened suddenly, illuminating the nebula. The coincident X-ray source was also observed to brighten fifty-fold as measured in Chandra observations obtained before and just after the optical outburst. The X-ray data are strong evidence that the probable cause of the outburst is the sudden infall of matter onto the surface of the star from an orbiting disk of gas.

The coupling of the magnetic field of the star and the magnetic field of its circumstellar disk regulates the inflow of gas from the disk onto the star. This slow, steady inflow suddenly can become much more rapid if a large amount of gas accumulates in the disk, and the disk and the star are rotating at different rates.

The differing rotation rates can twist and shear the magnetic field, storing up energy. This energy is eventually released in an energetic, X-ray producing outburst as the magnetic field violently rearranges back to a more stable state. During this period, a large amount of gas can fall onto the star, producing the observed optical and infrared outburst.

A new buildup of gas in the disk could lead to a new outburst in the future. Such a scenario may explain why the brightness of McNeil's Nebula appears to vary with time. It appears in optical images taken of this region of Orion in the 1960s, but is absent from images taken in the 1950s and 1990s.

NASA's Marshall Space Flight Center in Huntsville, Ala., manages the Chandra program for NASA. (NASA/CXC/RIT/J. Kastner et al.)


Story Source:

The above story is based on materials provided by NASA/Marshall Space Flight Center. Note: Materials may be edited for content and length.


Cite This Page:

NASA/Marshall Space Flight Center. "Chandra Sheds New Light On McNeil's Nebula." ScienceDaily. ScienceDaily, 29 July 2004. <www.sciencedaily.com/releases/2004/07/040729094140.htm>.
NASA/Marshall Space Flight Center. (2004, July 29). Chandra Sheds New Light On McNeil's Nebula. ScienceDaily. Retrieved September 3, 2014 from www.sciencedaily.com/releases/2004/07/040729094140.htm
NASA/Marshall Space Flight Center. "Chandra Sheds New Light On McNeil's Nebula." ScienceDaily. www.sciencedaily.com/releases/2004/07/040729094140.htm (accessed September 3, 2014).

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