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Heber, Ulrich; Geier, Stephan; Gaensicke, Boris (2012)
Publisher: EDP Sciences
Journal: EPJ Web of Conferences
Languages: English
Types: Article
Subjects: Astrophysics - Solar and Stellar Astrophysics, QC, Physics, QC1-999

Classified by OpenAIRE into

arxiv: Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Earth and Planetary Astrophysics
Research into hot subdwarf stars is progressing rapidly. We present recent important discoveries. First we review the knowledge about magnetic fields in hot subdwarfs and highlight the first detection of a highly-magnetic, helium-rich sdO star. We briefly summarize recent discoveries based on Kepler light curves and finally introduce the closest known sdB+WD binary discovered by the MUCHFUSS project and discuss its relevance as a progenitor of a double-detonation type Ia supernova.
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    • [1] Heber, U., ARAA 47, (2009) 211
    • [2] Geier, S., these proceedings, (2012)
    • [3] Kilkenny, D., Jeffery, C.S., & Koen, C., Fifth Meeting on Hot Subdwarf Stars and Related Objects (ASPC 452, San Francisco, 2012)
    • [4] Elkin, V.G., A&A 312, (1996) L5
    • [5] Elkin, V.G., Contributions of the Astronomical Observatory Skalnate Pleso 27, (1998) 452
    • [6] O'Toole, S.J., Jordan, S., Friedrich, S., & Heber, U., A&A 437, (2005) 227
    • [7] Chountonov, G., & Geier, S., APSC 452, (2012) 93
    • [8] Petit, P., Van Grootel, V., Bagnulo, S., et al., ASPC 452, (2012) 87
    • [9] Mathys, G., Hubrig, S., Mason, E., et al., Astronomische Nachrichten 333, (2012) 30
    • [10] Landstreet, J.D., Bagnulo, S., Fossati, L., Jordan, S., & O'Toole, S.J., A&A 541, (2012) A100
    • [11] Gaensicke, B. et al. 2012, in prep.
    • [12] Østensen, R.H., Silvotti, R., Charpinet, S., et al., MNRAS 414, (2011) 2860
    • [13] Bloemen, S., Marsh, T.R., Østensen, R.H., et al., MNRAS 410, (2011) 1787
    • [14] Han, Z., Podsiadlowski, P., Maxted, P.F.L., & Marsh, T.R., MNRAS 341,(2003) 669
    • [15] Geier, S., Hirsch, H., Tillich, A., et al., A&A 530, (2011) A28
    • [16] Geier, S., Schaffenroth, V., Drechsel, H., et al., ApJL 731, (2011) L22
    • [17] Geier, S., Schaffenroth, V., Hirsch, H., et al., ASPC 452, (2012) 129
    • [18] Beuermann, K., Dreizler, S., Hessman, F.V., & Deller, J., A&A 543, (2012) A138
    • [19] Vennes, S., Kawka, A., & Németh, P., MNRAS 410, (2011) 2095
    • [20] Geier, S., Marsh, T.R., Dunlap, B.H., et al., arXiv:1209.4740 (2012)
    • [21] Vennes, S., Kawka, A., O'Toole, S.J., Nemeth, P., & Burton, D., arXiv:1210.1512 (2012)
    • [22] Fink, M., Röpke, F.K., Hillebrandt, W., et al., A&A 514, (2010) A53
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