Publications · Joseph Cassinelli

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• The First Direct Measurement of an Early B Supergiant X-ray Source Electron Density

  Waldron, W., Cassinelli, J., Miller, N., Schlegel, E., 2012
  Conference Proceedings in "American Astronomical Society, AAS Meeting #219, #224.02" Pages
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• X-Ray Emission Line Profiles from Wind Clump Bow Shocks in Massive Stars

  Ignace, R., Waldron, W., Cassinelli, J., Burke, A., 2012
  The Astrophysical Journal, Vol. 750, Pages 40
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• X-ray Emissions from Clump Bowshocks in Massive Star Winds

  Ignace, R., Waldron, W., Cassinelli, J., 2012
  Conference Proceedings in "American Astronomical Society, AAS Meeting #219, #224.01" Pages
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• Linear Polarization Light Curves of Oblique Magnetic Rotators

  Ignace, R., Hole, K., Cassinelli, J., Henson, G., 2011
  Conference Proceedings in "American Astronomical Society, AAS Meeting #218, #121.06" Pages 12106
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• Time-dependent behavior of linear polarization in unresolved photospheres, with applications for the Hanle effect

  Ignace, R., Hole, K., Cassinelli, J., Henson, G., 2011
  Astronomy and Astrophysics, Vol. 530, Pages 82
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• X-ray emission from massive stars with magnetic fields

  Oskinova, L., Hamann, W., Cassinelli, J., Brown, J., Todt, H., 2011
  Astronomische Nachrichten, Vol. 332, Pages 988
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• A Multiphase Suzaku Study of X-rays from τ Sco

  Ignace, R., Oskinova, L., Jardine, M., Cassinelli, J., Cohen, D., et al., 2010
  The Astrophysical Journal, Vol. 721, Pages 1412-1420
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• The Importance of XUV Radiation as a Solution to the P V Mass Loss Rate Discrepancy in O Stars

  Waldron, W., Cassinelli, J., 2010
  The Astrophysical Journal Letters, Vol. 711, Pages L30-L34
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• Highly Accelerated Diamagnetic Plasmoids: A New X-Ray Production Mechanism for OB Stellar Winds

  Waldron, W., Cassinelli, J., 2009
  The Astrophysical Journal Letters, Vol. 692, Pages L76-L79
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• Polarization variability arising from clumps in the winds of Wolf-Rayet stars

  Li, Q., Cassinelli, J., Brown, J., Ignace, R., 2009
  Research in Astronomy and Astrophysics, Vol. 9, Pages 558-576
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