... Microvariability of Line Profiles in the Spectra of OB Stars: Ori A A. F. Kholtygin1* , T. E. Burlakova 1 2, 3 , S. N. Fabrika3, G. G. Valyavin2, 3 ,and M. V. Yushkin3 3 Sobolev Astronomical Institute, St. Petersburg State University, Bibliotechnaya pl. ... The dynamical wavelet spectrum of the profile variations reveals large-scale components in the interval 25-50 km/s that move within the -V sin I to V sin i band for the primary star of the system, Aa1 , with a band crossing time of 4h -5h . ...

... We explore the structures immediately surrounding the intermediate-mass young stellar object R Mon with bispec- trum speckle interferometry, conventional near-infrared imaging and by analyzing optical HST archive data. Our near-infrared speckle images with unprecedented diffraction-limited resolution of 55 mas (44 AU; H -band) and 76 mas (61 AU; K -band) represent the highest resolution R Mon images obtained so far and exhibit previously unseen complex structures. ... The features 1­5 are marked. ...