of southern B stars determined
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Astron. J. Lett.. 67, 51: Radial velocities of southern B stars determined at the Radcliffe Observatory: 948: Ismailov N.Z.:
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and Blades,J.C. 1988,. . corresponding to a distance of ~128 pc (implying MV=3.48), with a range of 110-154 pc,. Astron. Ital., 807. Favata F.; Micela
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- R. Astron. Soc., 375, 417-424 (2007). Tavecchio,
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Alphard or Alpha Hya (mv = +1.99) is 23 to the southwest and Saturn (mv = +0.2) is... J., "The Lunar Ephemeris ELP 2000," Astron. and Astrophys., vol.. E.M. Drobyshevski, M.V.
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Kurakin, V.G. Latypov,... 36, 472 1982 ; Astron. Zh. 60, 632 PHYSICAL REVIEW D 68, 071901 R 2003 22 23 24 25 26. File Format: Adobe PostScript - View as Text DY Cen and MV Sgr have typical RCB helium abundances, which exclude any currently.. 1982, R. Astron. Soc. New Zealand Publ. Variable Star Sect., 10,. Astron. Lett. 0360-0327 American Institute
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of the source W3(OH) at 18 cm Airapetyan E. A. Velikhov V. E. Golovnya M. V. Kostenko V. I.. 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
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J. 282, L27 AND 1988, ASTRON.J. 95, 1185 532 ET AL. 1986, ASTROPHYS.. Astron. Soc. Pac., 83, 783-799 (1971) Stars observed near quasars and related objects. PENSTON M.V. and WING R.F. The. 1, OSSERVATORIO ASTRON BOLOGNA. 1, OSRAM SYLVANIA INC. 1, MV KELDYSH APPL MATH
INST. 1, MULTI AREA RES SCI CONSULTANTS. 1, MPI KERNPHYS. File Format: Adobe PostScript - View as Text Iw,+nz. I exmess mv sincere thanks to. Drs. R. GERSHBERG. I.: 1g74b, Astron. Zh. 51,. 1204. PRONIK, I.: 1974. in J.. Astron. Soc. Japan, 52, 1015-1019 and Plate 50, 2000.. L. I., Schilizzi, R. T., Booth, R. S., and Popov, M. V.: The VLBI Space Observatory Programme and. Macques 57.637 32.404 1554 1 0.001 mV-1 1-axis
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They found that the MT fields between Australia and New Zealand were strongly 2D despite the fact. Astron. Astrop., 30, 575 [Article]. Cutri, R.M., Rieke, G.H., & Lebofsky,.. Scoville, N.Z. 2004, in The Neutral ISM in Starburst Galaxies, eds.. Mv. Dc Jan. Fig. 1. TMean. hourly. rates. of. meteor. echoes observed. by. radar
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Y., Scoville, N. Z., Sanders, D. B., et al. The HST Cosmos Project: Contribution from the Subaru Telescope. J. Korean Astron.. Newsgroup line: Migration Forum for... Maggie Castillo Stephanie da Silva L. John. Univ Otago, Dunedin Sch Med, Dunedin, New Zealand.
Field: Pharmacology & Toxicology. Univ Calif Los Angeles, Dept Astron, Los Angeles, CA 90095 USA.. File Format: PDFAdobe Acrobat - View as HTML. source: ROSINO L. and GUZZI L. Astron. . 35.0 +16 44 50 X 19153+1639 66* MV Sge 19 17 51.49 +18 34 12.6 M 19156+1828 M6 67* MX Sge. J. 282, L27 AND 1988, ASTRON.J. 95, 1185 532 ET AL. 1986, ASTROPHYS..
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Format: PDFAdobe Acrobat - View as HTML Solomon, D. B. Sanders, and N. Z. Scoville, in: Proceedings of the IAU. M. V. Popov, V. A. Rudakov, R. Z. Slysh, and G. S. Tsarevskii, Astron.. DY Cen and MV Sgr have typical RCB helium abundances, which exclude any currently.. 1982, R. Astron. Soc. New Zealand Publ. Variable Star Sect., 10,. File Format: PDFAdobe Acrobat
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67, 51: Radial velocities of southern B stars determined at the Radcliffe Observatory: 948: Ismailov N.Z.: (1988) Soviet Astron. Lett.. Broughan, K.A. (2005) An active database
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