Reference Type | Journal (article/letter/editorial) |
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Title | Why are accreting T Tauri stars observed to be less luminous in X-rays than non-accretors? |
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Journal | Monthly Notices of the Royal Astronomical Society: Letters |
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Authors | Gregory, S. G. | Author |
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Wood, K. | Author |
Jardine, M. | Author |
Year | 2007 (July 1) | Volume | 379 |
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Publisher | Oxford University Press (OUP) |
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DOI | doi:10.1111/j.1745-3933.2007.00328.xSearch in ResearchGate |
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| Generate Citation Formats |
Mindat Ref. ID | 3600557 | Long-form Identifier | mindat:1:5:3600557:6 |
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GUID | 0 |
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Full Reference | Gregory, S. G., Wood, K., Jardine, M. (2007) Why are accreting T Tauri stars observed to be less luminous in X-rays than non-accretors?. Monthly Notices of the Royal Astronomical Society: Letters, 379. doi:10.1111/j.1745-3933.2007.00328.x |
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Plain Text | Gregory, S. G., Wood, K., Jardine, M. (2007) Why are accreting T Tauri stars observed to be less luminous in X-rays than non-accretors?. Monthly Notices of the Royal Astronomical Society: Letters, 379. doi:10.1111/j.1745-3933.2007.00328.x |
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In | (2007) Monthly Notices of the Royal Astronomical Society: Letters Vol. 379. Oxford University Press (OUP) |
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