101![Rapid formation of large dust grains in the luminous supernova SN 2010jl Christa Gall1,2,3, Jens Hjorth2 , Darach Watson2, Eli Dwek3 , Justyn R. Maund4,2 , Ori Fox5 , Giorgos Leloudas6,2, Daniele Malesani2 & Avril C. Day Rapid formation of large dust grains in the luminous supernova SN 2010jl Christa Gall1,2,3, Jens Hjorth2 , Darach Watson2, Eli Dwek3 , Justyn R. Maund4,2 , Ori Fox5 , Giorgos Leloudas6,2, Daniele Malesani2 & Avril C. Day](https://www.pdfsearch.io/img/b469102b0c00d848db640a4eed02b311.jpg) | Add to Reading ListSource URL: www.eso.orgLanguage: English - Date: 2014-06-13 06:02:28
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102![The Astrophysical Journal, 627:534–539, 2005 July 1 # 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A. TRANSIT LIGHT-CURVE SIGNATURES OF ARTIFICIAL OBJECTS Luc F. A. Arnold Observatoire d The Astrophysical Journal, 627:534–539, 2005 July 1 # 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A. TRANSIT LIGHT-CURVE SIGNATURES OF ARTIFICIAL OBJECTS Luc F. A. Arnold Observatoire d](https://www.pdfsearch.io/img/e639a26f580c5168e72cd284c9cf36d6.jpg) | Add to Reading ListSource URL: www.obs-hp.frLanguage: English - Date: 2007-05-21 18:10:08
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103![6 · Explosive and Whirling Nebulæ ne of the most surprising triumphs of celestial O photography was Professor Keeler’s discovery, in 1899, that the great majority of the nebulæ have 6 · Explosive and Whirling Nebulæ ne of the most surprising triumphs of celestial O photography was Professor Keeler’s discovery, in 1899, that the great majority of the nebulæ have](https://www.pdfsearch.io/img/510d106152bc2fc26ccbcf6f6508a892.jpg) | Add to Reading ListSource URL: www.tug.orgLanguage: English - Date: 2003-03-17 16:40:22
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104![1. Das neue IfGI-Logo 1.6 Logovarianten Subsetting of Spatio-Temporal Objects Logo für den Einsatz in internationalen bzw. 1. Das neue IfGI-Logo 1.6 Logovarianten Subsetting of Spatio-Temporal Objects Logo für den Einsatz in internationalen bzw.](https://www.pdfsearch.io/img/e4ab64eb9f451ba8a07aa5df727c0a45.jpg) | Add to Reading ListSource URL: cran.skazkaforyou.comLanguage: English - Date: 2015-02-19 19:31:13
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105![The Astrophysical Journal, 590:906–916, 2003 June 20 # 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A. THE IMPACT OF IONIZING STARS ON THE DIFFUSE INTERSTELLAR MEDIUM: A SWEPT-UP SHELL A The Astrophysical Journal, 590:906–916, 2003 June 20 # 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A. THE IMPACT OF IONIZING STARS ON THE DIFFUSE INTERSTELLAR MEDIUM: A SWEPT-UP SHELL A](https://www.pdfsearch.io/img/ee8a35e7c33b2fb42b992124b11d5fec.jpg) | Add to Reading ListSource URL: terryhancock.narya.netLanguage: English - Date: 2012-03-09 18:01:21
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106![ELAINE CAMERON-WEIR NEW YORK by Natalie Bell In Elaine Cameron-Weir’s solo show without true bazaars, objects occupy measurable space while holding critically indifferent positions [RAMIKEN CRUCIBLE; may 8 - june 19, 2 ELAINE CAMERON-WEIR NEW YORK by Natalie Bell In Elaine Cameron-Weir’s solo show without true bazaars, objects occupy measurable space while holding critically indifferent positions [RAMIKEN CRUCIBLE; may 8 - june 19, 2](https://www.pdfsearch.io/img/8fec48eea18f118d06d3f5b8f07665ed.jpg) | Add to Reading ListSource URL: www.ramikencrucible.comLanguage: English - Date: 2012-01-27 19:07:23
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107![e.g., the 10-9, 2.429t-tm, observed in other high excitation objects such as Wolf-Rayet stars (Aitken et al., 1982, Monthly Notices of the Royal Astronomical Society, 200, 698) are not present in our spectrum of the nova e.g., the 10-9, 2.429t-tm, observed in other high excitation objects such as Wolf-Rayet stars (Aitken et al., 1982, Monthly Notices of the Royal Astronomical Society, 200, 698) are not present in our spectrum of the nova](https://www.pdfsearch.io/img/9cea4765cb4134eac731317fca2b206d.jpg) | Add to Reading ListSource URL: www.eso.orgLanguage: English - Date: 2009-06-05 10:39:39
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108![Measuring Black Hole Masses in Nearby Galaxies with Laser Guide Star Adaptive Optics Claire Max Anne Medling Measuring Black Hole Masses in Nearby Galaxies with Laser Guide Star Adaptive Optics Claire Max Anne Medling](https://www.pdfsearch.io/img/bdb08c9abed0ee6238785fc646440788.jpg) | Add to Reading ListSource URL: www.noao.eduLanguage: English - Date: 2009-07-20 15:10:28
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109![General Description Guidelines Galaxies Did you use direct or averted vision? What is the overall shape? Is the core noticeable, compact, stellar ? Can structure be seen in the galaxy, mottling, General Description Guidelines Galaxies Did you use direct or averted vision? What is the overall shape? Is the core noticeable, compact, stellar ? Can structure be seen in the galaxy, mottling,](https://www.pdfsearch.io/img/bd1a3a7af2d422d549500f095e755b1b.jpg) | Add to Reading ListSource URL: www.astronomylogs.comLanguage: English - Date: 2009-07-19 17:08:06
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110![IAC-14.A6.1.1 CAPABILITY OF A SPACE-BASED SPACE SURVEILLANCE SYSTEM TO DETECT AND TRACK OBJECTS IN GEO, MEO AND LEO ORBITS Jiri Silha1,2, Thomas Schildknecht1, Andreas Hinze1 Astronomical Institute, University of Bern, C IAC-14.A6.1.1 CAPABILITY OF A SPACE-BASED SPACE SURVEILLANCE SYSTEM TO DETECT AND TRACK OBJECTS IN GEO, MEO AND LEO ORBITS Jiri Silha1,2, Thomas Schildknecht1, Andreas Hinze1 Astronomical Institute, University of Bern, C](https://www.pdfsearch.io/img/72c8b3a4b445c30f01706e9573146d07.jpg) | Add to Reading ListSource URL: aiuws.unibe.chLanguage: English - Date: 2014-10-27 05:36:42
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