Circumnuclear regions of different BPT types in star-forming MaNGA galaxies: AGN detectability of the intermediate type; (2) INT, the central area of radiation of the intermediate type; (3) SF+INT, the
inner Hints of a rotating spiral structure in the innermost regions around IRC+10216Quintana-Lacaci, G.,
Agundez, M.,
Velilla Prieto, L.,
Castro-Carrizo, A.,
Marcelino, N.,
Cabezas, C.,
Pena, I.,
Alonso, J. L.,
Zuniga, J.,
Cernicharo, José,
Requena, A.,
Bastida, A.,
Kalugina, Yulia N.,
Lique, Francois,
Guelin, M. presents an
inner minimum of 27 AU. In the case of the torus, the outer
radius is 73 AU. The kinematics
SINUSOIDAL VELAROIDAL SHELL - NUMERICAL MODELLING OF THE NONLINEAR BUCKLING RESISTANCE and the force nonlinearity. The nonlinearity, applied to a sinusoidal velaroidal shell with the
inner radius r(0
The thickness of accretion α-disks: Theory and observations in these systems (up to h/R ≈ 0.25, where h is the disk half-thickness and R its
radius), while standard α
Asynchronous iterations of HSS method for non-Hermitian linear systems is theoretically ensured both under classical spectral
radius bound and, then, for a classical class of matrix
Dynamic state of columnar structures formed on the basis of carbon nanotori with a small
inner radius. Using this potential, a characteristic fragment of a columnar crystal