BY Cam: There and Back

Bypass to Turbulence in Hydrodynamic Accretion Disks: An Eigenvalue Approach

Bypass to Turbulence in Hydrodynamic Accretion: Lagrangian Analysis of Energy Growth

Byurakan Astrophysical Observatory

Byurakan spectral sky surveys. Blue stellar objects in the strip at δ = +47°

BZ Cam during its 1999/2000 optical low state

BZ-MC-BP Model for Jet Production from Black Hole Accretion Disc

BZBJ1058+5628: a new quasi-periodic BL Lac

B[e] phenomenon extending to lower luminosities in the Magellanic Clouds.

B[e] stars at the highest angular resolution: the case of HD87643

B[e] stars. VI. MWC 297 = IRAS 18250-0351

B[e] stars. VII. MWC 17

B[e] stars. VIII. MWC 342

B[e] supergiants: What is their evolutionary status?

B^F Theory and Flat Spacetimes

B_gg revisited: The environments of low-excitation radio galaxies and unified models