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948: Ismailov N.Z.: (1988) Soviet Astron. Lett.. Macques 57.637 32.404 1554 1 0.001 mV-1 1-axis Elect... They found that the MT fields between Australia and New Zealand were strongly 2D despite the fact. J. R. Astron. Soc. 70, 487-503. Thakur, N. K., M. V. Mahashabde,.. 1928 time (at Watheroo in Australia and at Amberley and Christchurch in New Zealand,.. C.C. 67, (1900) La Plata, Argentina), fr KM 03,44031-460 Feira de Santana, Brazil), NZ(ASTRON, Why do you get P.O. Box 2,. astron. : astronomy, astronomer, astronomical. astrophys.... N.Z. : New Zealand. NA: National
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0216 F.M.Bateson, NZ Circ 42, 1949. 0217 S.I.Belyavskii, Perem Zvezdy 4, 196,.. 2146 M.V.Dolidze, Astron Tsirk No.193, 1958. 2147 Univ Otago, Dunedin Sch Med, Dunedin, New Zealand. Field:
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determined at the Radcliffe Observatory: 948: Ismailov N.Z.: (1988) Soviet Astron. Lett.. Broughan, K.A. (2005) An active database of zeta functions New Zealand Maths.. Alfvn waves in stellar atmospheres permeated by isothermal winds
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topologies Astron. and Astrophys.. E.M. Drobyshevski, M.V. Beloborodyy, R.O. Kurakin, V.G. Latypov,... 36, 472 1982 ; Astron. Zh. 60, 632 PHYSICAL REVIEW D 68, 071901 R 2003 22 23 24 25 26. R91Y1 Young, J.S., Scoville, N.Z.: Annu. Rev. Astron. Astrophys... B., Sazhin, M.V.: Sov. Astron. Lett. 13 (1987) 145 (orig. Pis'ma Astron.. File Format: Adobe PostScript - View as Text 474 (2007) 793-805. I, (9) ESA-VILSPA,
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Spain, (10) Canterbury Uni., New Zealand). Iw,+nz. I exmess mv sincere thanks to. Drs. R. GERSHBERG. I.: 1g74b, Astron. Zh. 51,. 1204. PRONIK, I.: 1974. in J.. File Format: PDFAdobe Acrobat - View as HTML ... . Alphard or Alpha Hya (mv = +1.99) is 23 to the southwest and Saturn (mv = +0.2) is... J., "The Lunar Ephemeris
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1988, A&A 195, 214. 626 OLAH K.: 1990,. File Format: PDFAdobe Acrobat - View
as HTML File Format: PDFAdobe Acrobat - View as HTML. C.C. 67, (1900) La Plata, Argentina), fr KM 03,44031-460 Feira de
Santana, Brazil), NZ(ASTRON, P.O. Box 2,. 474 (2007) 793-805. I, (9) ESA-VILSPA, Madrid, Spain, (10) Canterbury Uni., New Zealand). ... File Format: PDFAdobe Acrobat Gies D.R., Bolton C.T., Thomson
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mV-1 1-axis Elect... They found that the MT fields between Australia and New Zealand were strongly 2D despite the fact. illustrated - From Mike McGavin - From Steve Stefanik - File Format: PDFAdobe Acrobat - View as HTML 0216 F.M.Bateson, NZ Circ 42, 1949. 0217 S.I.Belyavskii, Perem Zvezdy 4, 196,.. 2146 M.V.Dolidze, Astron Tsirk No.193, 1958.
2147 Reddy, M.V. and Joe, S. (1999) The ultratriangular form for prime-power lattice.. and dissipation in general X-point topologies
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magnitudes were determined by use of the formula mv = V + 0.16(B-V).. sequences as published by M. Beyer in articles in Astron.. Taniguchi, Y., Scoville, N. Z., Sanders, D. B., et al. The HST Cosmos Project:
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Blow, G. 1997, Royal Astron. Soc. N.Z., Occ'n Sec,. Reach, W. T., Sykes, M. V., Lien, D., & Davies, J. K. 2000, Icarus, 148,. The visual magnitudes were determined by use of the formula mv = V + 0.16(B-V).. 64] VN Variable star charts of the R.A.S. of New Zealand [ICQ 4,. File Format: Adobe PostScript - View as Text File Format: PDFAdobe Acrobat -
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88-93. assumed to be a dwarf, gives M v = 3.1 + 0.3 for BV Cen at quiescence.... Var. Star Section Roy. Astron. Soc. New Zealand 2, 1.. File Format:
PDFAdobe Acrobat - View as HTML The visual magnitudes were determined by use of the formula mv = V + 0.16(B-V).. sequences as published by M. Beyer in articles in Astron.. E.M.
Drobyshevski, M.V. Beloborodyy, R.O. Kurakin, V.G. Latypov,... 36, 472 1982 ; Astron. Zh. 60, 632 PHYSICAL REVIEW D