Authors:
MENSHCHIKOV AB
BALEGA YY
OSTERBART R
WEIGELT G
Citation: Ab. Menshchikov et al., HIGH-RESOLUTION BISPECTRUM SPECKLE INTERFEROMETRY AND 2-DIMENSIONAL RADIATIVE-TRANSFER MODELING OF THE RED-RECTANGLE, New astronomy (Online), 3(8), 1998, pp. 601-617
Citation: A. Cadez et al., LINE EMISSION FROM ACCRETION DISCS AROUND BLACK-HOLES - THE ANALYTIC APPROACH, New astronomy (Online), 3(8), 1998, pp. 647-654
Authors:
DESERT FX
BENOIT A
GAERTNER S
BERNARD JP
CORON N
DELABROUILLE J
DEMARCILLAC P
GIARD M
LAMARRE JM
LEFLOCH B
PUGET JL
SIRBI A
Citation: Fx. Desert et al., OBSERVATIONS OF THE SUNYAEV-ZELDOVICH EFFECT AT HIGH ANGULAR RESOLUTION TOWARDS THE GALAXY CLUSTERS A665, A2163 AND CL0016+16, New astronomy (Online), 3(8), 1998, pp. 655-669
Citation: A. Hujeirat et Hw. Yorke, ON THE MHD STRUCTURE OF THE SOLAR TACHOCLINE - STEADY AND DYNAMICAL SOLUTIONS, New astronomy (Online), 3(8), 1998, pp. 671-685
Authors:
MACFARLAND T
COUCHMAN HMP
PEARCE FR
PICHLMEIER J
Citation: T. Macfarland et al., A NEW PARALLEL (PM)-M-3 CODE FOR VERY LARGE-SCALE COSMOLOGICAL SIMULATIONS, New astronomy (Online), 3(8), 1998, pp. 687-705
Authors:
VANBEVEREN D
DEDONDER E
VANBEVER J
VANRENSBERGEN W
DELOORE C
Citation: D. Vanbeveren et al., THE WR AND O-TYPE STAR POPULATION PREDICTED BY MASSIVE STAR EVOLUTIONARY SYNTHESIS, New astronomy (Online), 3(7), 1998, pp. 443-492
Citation: Bd. Fields et al., MASSIVE COMPACT HALO OBJECTS VIEWED FROM A COSMOLOGICAL PERSPECTIVE -CONTRIBUTION TO THE BARYONIC MASS DENSITY OF THE UNIVERSE, New astronomy, 3(6), 1998, pp. 347-361
Citation: Sa. Bonometto et E. Pierpaoli, MIXED MODELS WITH N-GREATER-THAN-1 AND LARGE-SCALE STRUCTURE CONSTRAINTS, New astronomy, 3(6), 1998, pp. 391-409
Citation: Sp. Boughn et al., CORRELATIONS BETWEEN THE COSMIC X-RAY AND MICROWAVE BACKGROUNDS - CONSTRAINTS ON A COSMOLOGICAL CONSTANT, New astronomy, 3(5), 1998, pp. 275-291
Citation: Sp. Boughn et al., CORRELATIONS BETWEEN THE COSMIC X-RAY AND MICROWAVE BACKGROUNDS - CONSTRAINTS ON A COSMOLOGICAL CONSTANT, New astronomy, 3(5), 1998, pp. 275-291