1. Superflares on solar-type stars.

    Nature 485(7399):478 (2012) PMID 22622572

    Solar flares are caused by the sudden release of magnetic energy stored near sunspots. They release 10(29) to 10(32) ergs of energy on a timescale of hours. Similar flares have been observed on many stars, with larger 'superflares' seen on a variety of stars, some of which are rapidly rotating a...
  2. Superflares on solar-type stars.

    Nature 485(7399):478 (2012) PMID 22622572

    Solar flares are caused by the sudden release of magnetic energy stored near sunspots. They release 10(29) to 10(32) ergs of energy on a timescale of hours. Similar flares have been observed on many stars, with larger 'superflares' seen on a variety of stars, some of which are rapidly rotating a...
  3. Structure in the early afterglow light curve of the gamma-ray burst of 29 March 2003.

    Nature 423(6942):843 (2003) PMID 12815423

    Gamma-ray bursts (GRBs) are energetic explosions that for 0.01-100 s are the brightest gamma-ray sources in the sky. Observations of the early evolution of afterglows are expected to provide clues about the nature of the bursts, but their rapid fading has hampered such studies; some recent rapid...
  4. Structure in the early afterglow light curve of the gamma-ray burst of 29 March 2003.

    Nature 423(6942):843 (2003) PMID 12815423

    Gamma-ray bursts (GRBs) are energetic explosions that for 0.01-100 s are the brightest gamma-ray sources in the sky. Observations of the early evolution of afterglows are expected to provide clues about the nature of the bursts, but their rapid fading has hampered such studies; some recent rapid...