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Cited article:

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Monthly Notices of the Royal Astronomical Society 376 (3) 1145 (2007)
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Dust Morphology and Composition in FU Orionis Systems

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X‐Ray Study of Herbig Ae/Be Stars

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Does the 3.3 Micron Polycyclic Aromatic Hydrocarbon Emission Feature Require Ultraviolet Excitation?

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The stellar composition of the star formation region CMa R1 - III. A new outburst of the Be star component in Z CMa

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