| Reference Type | Journal (article/letter/editorial) |
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| Title | X-RAY SCALING RELATION IN EARLY-TYPE GALAXIES: DARK MATTER AS A PRIMARY FACTOR IN RETAINING HOT GAS |
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| Journal | The Astrophysical Journal |
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| Authors | Kim, Dong-Woo | Author |
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| Fabbiano, Giuseppina | Author |
| Year | 2013 (October 7) | Volume | 776 |
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| Issue | 2 |
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| Publisher | IOP Publishing |
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| DOI | doi:10.1088/0004-637x/776/2/116Search in ResearchGate |
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| Generate Citation Formats |
| Mindat Ref. ID | 3388950 | Long-form Identifier | mindat:1:5:3388950:6 |
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| GUID | 0 |
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| Full Reference | Kim, Dong-Woo, Fabbiano, Giuseppina (2013) X-RAY SCALING RELATION IN EARLY-TYPE GALAXIES: DARK MATTER AS A PRIMARY FACTOR IN RETAINING HOT GAS. The Astrophysical Journal, 776 (2). 116pp. doi:10.1088/0004-637x/776/2/116 |
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| Plain Text | Kim, Dong-Woo, Fabbiano, Giuseppina (2013) X-RAY SCALING RELATION IN EARLY-TYPE GALAXIES: DARK MATTER AS A PRIMARY FACTOR IN RETAINING HOT GAS. The Astrophysical Journal, 776 (2). 116pp. doi:10.1088/0004-637x/776/2/116 |
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| In | (2013, October) The Astrophysical Journal Vol. 776 (2) IOP Publishing |
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