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pro vyhledávání: '"H. L. Helfer"'
Autor:
H. L. Helfer
Publikováno v:
The Astrophysical Journal. 880:73
Publikováno v:
The Astrophysical Journal. 534:944-966
We present the results of a linearized perturbation analysis for the models of cataclysmic variable (CV) disks and their boundary layers (BLs), discussed in a previous companion paper. For the case of large-scale, azimuthal oscillations in the BL, we
Publikováno v:
The Astrophysical Journal. 534:934-943
We consider numerical models of accretion disks and boundary layers (BLs) around white dwarfs in cataclysmic variables (CVs). Our models include the effects of the radial viscous force and are created using the realistic OPAL opacities. We present th
Autor:
M. P. Savedoff, H. L. Helfer
Publikováno v:
Astrophysics and Space Science. 188:299-320
The efficiency of the anti-proton (pBAR) production in interstellar clouds is increased by a factor ≳50 when the engendering cosmic-ray protons (CRs) experience diffusive acceleration by shocks. One can represent the pBAR/p observations by a conven
A Model for Quasi-periodic Oscillations in Cataclysmic VariablesBased on Boundary Layer Oscillations
Publikováno v:
The Astrophysical Journal. 508:L159-L161
We have performed a linearized perturbation analysis of the disk and boundary layer (BL) in a cataclysmic variable. In the BL, we find a triplet of large-scale, torsional oscillation modes consisting primarily of perturbations of the azimuthal veloci
Publikováno v:
The Astrophysical Journal. 365:252
M8 est une nebuleuse emissive contenant une region H II a brillance de surface elevee, Hourglass, en direction de laquelle de nombreuses sources IR compactes ont ete detectees. Les images IR multilongueurs d'onde et a haute resolution spatiale de M8
Autor:
H. L. Helfer, P. A. Jennens
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 172:681-694
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 209:209-214
VLA radio maps at 5-GHz of the G10.2-0.3 H II region in the W31 complex reveal an extended ionization ridge of dimensions 5.7 x 2.9 sq pc at an assumed distance of 7 kpc. In the ridge, 21 dense clumps have been found with characteristic emission meas
Autor:
H. L. Helfer, J. N. McMullin
Publikováno v:
Solar Physics. 53:471-488
The problem of predicting the radio emission from the quiet Sun for meter and decameter waves may be formulated in terms of a standard radiative transfer problem with conservative scattering. One may therefore avoid the numerical complications involv
Autor:
H. L. Helfer, P. A. Jennens
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 172:701-705