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Articles 1 - 18 of 18

Full-Text Articles in Physical Sciences and Mathematics

Croatian Symposium Of Chemistry And Macromolecular Chemistry, Otto Vogl, Zvonimir Janovic Dec 1995

Croatian Symposium Of Chemistry And Macromolecular Chemistry, Otto Vogl, Zvonimir Janovic

Otto Vogl

No abstract provided.


Polymer Science In Australia Iv. Universities In Victoria And Southern Australia, Otto Vogl, David Solomon, Ezio Rizzardo, Robert A. Shanks, David Williams Dec 1995

Polymer Science In Australia Iv. Universities In Victoria And Southern Australia, Otto Vogl, David Solomon, Ezio Rizzardo, Robert A. Shanks, David Williams

Otto Vogl

No abstract provided.


52. Bengt Ranby, Otto Vogl Dec 1995

52. Bengt Ranby, Otto Vogl

Otto Vogl

No abstract provided.


Reconstruction Of Solar Irradiance Since 1610: Implications For Climate Cbange, Judith Lean, Juerg Beer, Raymond S. Bradley Dec 1995

Reconstruction Of Solar Irradiance Since 1610: Implications For Climate Cbange, Judith Lean, Juerg Beer, Raymond S. Bradley

Raymond S Bradley

Solar total and ultraviolet (UV) irradiances are reconstructed annually from J610 to the present. This epoch ~ludes the Maunder Minimmn of anomalously low solar activi1}' (circa 1645-1115) and the subsequent increase to the high levels of the present Modem Maximum. In this reconstruction, the Schwabe (II-year) irradiaoce cycle and a longer term Variability component are determined separately, based on contemporary. solar and stellar monitoring. The correlation of reconstructed solar irradiance and Northern Hemisphere (NIl) surface temperature is 0.86 in the pre-industrial period from 1610 to 1800, implying a predominant solar influence. Extending this correlation to the present suggests that solar …


53. Takeo Saegusa, Otto Vogl Nov 1995

53. Takeo Saegusa, Otto Vogl

Otto Vogl

No abstract provided.


Extended Molecular Gas Distribution In Mrk 273 And Merger-Luminosity Evolution, Min S. Yun, N Z. Scoville Oct 1995

Extended Molecular Gas Distribution In Mrk 273 And Merger-Luminosity Evolution, Min S. Yun, N Z. Scoville

Min S. Yun

We present the first interferometric measurement of CO emission (θ ~ 2'') from the ultraluminous infrared galaxy Mrk 273. A total H2 mass of 3.6 × 1010 Msun is inferred from the CO observations, half of which belongs to an extended component with deconvolved size 5.1 × 2.5 kpc. In addition, an unresolved molecular gas complex is found to be coincident with the optical nucleus. The inferred H2 mass, size (R ~ 380 pc), and mean surface mass density (ΣH2 ≥ 4 × 104 Msun pc-3) of this complex, as well as the IR luminosity, are very similar to those …


54. Burkart Philipp, Otto Vogl, Ch. Wandrey Oct 1995

54. Burkart Philipp, Otto Vogl, Ch. Wandrey

Otto Vogl

No abstract provided.


55. Hermann Janeschitz-Kriegl, Otto Vogl, Anton Schausberger Sep 1995

55. Hermann Janeschitz-Kriegl, Otto Vogl, Anton Schausberger

Otto Vogl

No abstract provided.


56. Sir Geoffrey Allan, Otto Vogl, Shigeko Suzuki Aug 1995

56. Sir Geoffrey Allan, Otto Vogl, Shigeko Suzuki

Otto Vogl

No abstract provided.


57. Peter Plesch, Otto Vogl, Traudl Plesch Jul 1995

57. Peter Plesch, Otto Vogl, Traudl Plesch

Otto Vogl

No abstract provided.


58. Koichi Hatada, Otto Vogl, Michiko Hatada Jun 1995

58. Koichi Hatada, Otto Vogl, Michiko Hatada

Otto Vogl

No abstract provided.


59. Otto Kratky, 1902-1995, Otto Vogl, Josef Schurz May 1995

59. Otto Kratky, 1902-1995, Otto Vogl, Josef Schurz

Otto Vogl

No abstract provided.


Electron Scattering From 10b, A Cichocki, J Dubach, R S. Hicks, Gerald Alvin Peterson May 1995

Electron Scattering From 10b, A Cichocki, J Dubach, R S. Hicks, Gerald Alvin Peterson

Gerald Alvin Peterson

Electron scattering measurements have been made in order to determine the longitudinal and transverse form factors of low-lying level in 10B. With the exception of the broad 5.18 MeV level, results were obtained for all known levels up to 6.7 MeV. The measurements span the momentum transfer range q=0.48–2.58 fm-1. The primary objective of this work was to improve the data on the pure isovector M3 form factor of the 1.740 MeV excitation, the transform of which yields the 1p3/2 single-nucleon wave function. A Woods-Saxon potential was found to provide a much better representation of the data than the harmonic …


60. Teiji Tsuruta, Otto Vogl Apr 1995

60. Teiji Tsuruta, Otto Vogl

Otto Vogl

No abstract provided.


61. Marian Kryszewski, Otto Vogl Mar 1995

61. Marian Kryszewski, Otto Vogl

Otto Vogl

No abstract provided.


62. David M Solomon, Otto Vogl, Kenneth Ghiggino Feb 1995

62. David M Solomon, Otto Vogl, Kenneth Ghiggino

Otto Vogl

No abstract provided.


Extended Molecular Gas In Fsc 10214+4724, N Z. Scoville, Min S. Yun, R L. Brown, P A. Vanden Bout Jan 1995

Extended Molecular Gas In Fsc 10214+4724, N Z. Scoville, Min S. Yun, R L. Brown, P A. Vanden Bout

Min S. Yun

e report high resolution imaging of the CO (3-2) emission in the luminous infrared source FSC 10214+4724 at z = 2.2853. Maps at resolutions of 2farcs3 × 3farcs0 and 45-90 km s-1 show the CO emission peak coinciding with those of Hα and radio continuum. Two components are identified in the CO emission: an unresolved core and an extended source (~1farcs9 × 4farcs4)—elongated southeast-northwest. The implied size is 9 × 24 kpc for H0 = 75 km s-1 Mpc-1 and q0 = 0.5. The extent of the CO emission is significantly greater than that of either the optical or the …


63. Ivan Panayotov, Otto Vogl, Christo Tsvetanov Jan 1995

63. Ivan Panayotov, Otto Vogl, Christo Tsvetanov

Otto Vogl

No abstract provided.