SPIN DETERMINATION OF HIGHLY EXCITED NUCLEI FROM LIGHT PARTICLE EMISSION STUDIES

1980 ◽  
Vol 41 (C10) ◽  
pp. C10-217-C10-228
Author(s):  
D. Guerreau ◽  
R. Babinet
Keyword(s):  
Particle Emission ◽  
Light Particle ◽  
Excited Nuclei ◽  
Spin Determination ◽  
Emission Studies

Spin determination of deeply-bound hole states from ( $$\vec d$$ ,3He) reactions

1980 ◽  
Vol 297 (4) ◽  
pp. 307-309 ◽  
Author(s):  
A. Stuirbrink ◽  
G. J. Wagner ◽  
K. T. Kn�pfle ◽  
Liu Ken Pao ◽  
G. Mairle ◽  
...  
Keyword(s):  
Spin Determination

Determination of theQ-value dependence of charged particle emission in the40Ca+40Ca reaction at 10 MeV/nucleon

1980 ◽  
Vol 294 (2) ◽  
pp. 159-165 ◽  
Author(s):  
A. Ameaume ◽  
G. Bizard ◽  
J. L. Laville ◽  
M. Louvel ◽  
P. Colombani ◽  
...  
Keyword(s):  
Charged Particle ◽  
Particle Emission ◽  
Charged Particle Emission

Spin determination of the 12C + 12C resonance at Ec.m. = 6.25 MeV

1977 ◽  
Vol 67 (3) ◽  
pp. 262-264 ◽  
Author(s):  
W. Galster ◽  
W. Treu ◽  
P. Dück ◽  
H. Fröhlich ◽  
H. Voit
Keyword(s):  
Spin Determination

WISE data and sparse photometry used for shape reconstruction of asteroids

2015 ◽  
Vol 10 (S318) ◽  
pp. 170-176 ◽  
Author(s):  
Josef Ďurech ◽  
Josef Hanuš ◽  
Victor M. Alí-Lagoa ◽  
Marco Delbo ◽  
Dagmara A. Oszkiewicz
Keyword(s):  
Rotation Period ◽  
Shape Reconstruction ◽  
Physical Models ◽  
Inversion Method ◽  
Wide Field ◽  
Reflected Light ◽  
Space Data ◽  
Spin Determination ◽  
Infrared Survey

AbstractAsteroid disk-integrated sparse-in-time photometry can be used for determination of shapes and spin states of asteroids by the lightcurve inversion method. To clearly distinguish the correct solution of the rotation period from other minima in the parameter space, data with good photometric accuracy are needed. We show that if the low-quality sparse photometry obtained from ground-based astrometric surveys is combined with data from the Wide-field Infrared Survey Explorer (WISE) satellite, the correct rotation period can be successfully derived. Although WISE observed in mid-IR wavelengths, we show that for the period and spin determination, these data can be modelled as reflected light. The absolute fluxes are not required since only relative variation of the flux over the rotation is sufficient to determine the period. We also discuss the potential of combining all WISE data with the Lowell photometric database to create physical models of thousands of asteroids.

Prompt light particle emission in the 36Ar + 58Ni reaction at 95 MeV/nucleon

2000 ◽  
Vol 9 (3) ◽  
pp. 371-383 ◽  
Author(s):  
P. Pawłowski ◽  
◽  
B. Borderie ◽  
G. Auger ◽  
Ch.O. Bacri ◽  
...  
Keyword(s):  
Particle Emission ◽  
Light Particle

Light-particle emission in the reaction 32S + 27A1 AT 135 and 190 MeV

1981 ◽  
Vol 371 (3) ◽  
pp. 454-476 ◽  
Author(s):  
D. Pelte ◽  
U. Winkler ◽  
R. Novotny ◽  
H. Gräf
Keyword(s):  
Particle Emission ◽  
Light Particle
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