X線による古典新星の観測
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(131) ῎῍῏ῌ 1) Brahe T., 1573, De nova et nullius aevi memoria prius visa stella iam pridem anno a nato Christo 1572 mense novembri primium conspecta 2) Hess V. F., 1912, Phys. Z. 13, 1084 3) Duquennoy A., Mayor M., 1991, A&A 248, 485 4) Takei D., Tsujimoto M., Kitamoto S., Morii M., Ebisawa K., Maeda Y., Miller E. D., 2008, PASJ 60, S231 5) Tsujimoto M., Takei D., Drake J. J., Ness J.-U., Kitamoto S., 2009, PASJ 61, S69 6) Takei D., Tsujimoto M., Kitamoto S., Ness J.-U., Drake J. J., Takahashi H., Mukai K., 2009, ApJL 697, L54 7) Hachisu I., Kato M., 2005, ApJ 631, 1094 8) Hachisu I., Kato M., 2006, ApJS 167, 59 9) Hachisu I., Kato M., 2010, ApJ, 709, 680 10) Lloyd H. M., O’Brien T. J., Bode M. F., Predehl P., Schmitt J. H. M. M., Truemper J., Watson M. G., Pounds K. A., 1992, Nature 356, 222 11) Mukai K., Ishida M., 2001, ApJ 551, 1024 12) Nakano S., Kadota K., Waagen E., Swierczynski S., Komorous M., King R., Bortle J., 2007, IAU Circ. 8861, 2 13) Samus N. N., 2007, IAU Circ. 8863, 2 14) Drake J. J., et al., 2007, The Astronomer’s Telegram 1246, 1 15) Smith R. K., Brickhouse N. S., Liedahl D. A., Raymond J. C., 2001, ApJ 556, L91 16) Koyama K., Petre R., Gotthelf E. V., Hwang U., Matsuura M., Ozaki., M., Holt S. S., 1995, Nature 378, 255 17) Tatische# V., Hernanz M., 2007, ApJL 663, 101 18) Rupen M. P., Mioduszewski A. J., Sokoloski J. L., 2008,. 464. ApJ 688, 559 19) Krauss Hartman. M. I., Rupen M. P., Mioduszewski A. J., 2009, The Astronomer’s Telegram 2195, 1 20) Nakano S., et al., 2008, IAU Circ. 8934, 1 21) Samus N. N., 2008, IAU Circ. 8934, 2 22) Ibarra A., Kuulkers E., 2008, The Astronomer’s Telegram 1473, 1 23) Ibarra A., et al., 2008, The Astronomer’s Telegram 1478, 1 24) Page K. L., et al., 2010, MNRAS 401, 121 25) Hachisu I., Kato M., 2009, ApJL 694, L103 26) Kuulkers E., et al., 2008, The Astronomer’s Telegram 1480, 1. X-ray Observations of Classical Novae Dai TAKEI Department of Physics, Rikkyo University, 3ῌ34ῌ1 Nishi-Ikebukuro, Toshima-ku, Tokyo 171ῌ8501, Japan Abstract : Classical novae occur in binary systems consisting of a white dwarf and a late-type companion. Systematic studies with many samples are mandatory to elucidate the general picture of their evolutions, and X-ray observations are well-suited to understanding their nature. However, observing classical novae is di$cult because of their faintness and transient behavior. We have therefore conducted ToO observations with the Suzaku X-ray satellite, and have sought classical novae in archival data. In this article, we introduce our strategy and latest results on X-ray observations of classical novae.. ῍῏ῌῐ. 2010 ῎ 7 ῌ.
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