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" Tait, and was brought to the notice of this Association in 1871 by Sir William Thomson in his Presidential Address. The spectrum of the bright-line... "
The Observatory - Page 240
1910
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Chemical News and Journal of Industrial Science, Volume 64

1891 - 346 pages
...in 1871 by Sir William Thomson in his Presidential Address. The spectrum of the bright-line nebulae is certainly not such a spectrum as we should expect...meteorites would first show themselves — iron, sodium, magnesum, nickel, &c.— are not those which distinguish the nebular spectrum. On the contrary, this...
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Telegraphic Journal and Monthly Illustrated Review of Electrical ..., Volume 8

1891 - 680 pages
...in 1871 by Sir William Thomson in his prea dential address. The spectrum of the bright-line nebula; is certainly not such a spectrum as we should expect...strongest lines of the substances which in the case ot such meteorites would first show themselves— iron, sodium, magnesium, nickel, etc. — are not...
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Report of the Annual Meeting

British Association for the Advancement of Science - 1892 - 1146 pages
...in 1871 by Sir William Thomson in his Presidential Address. The spectrum of the bright-line nebulee is certainly not such a spectrum as we should expect...magnesium, nickel, &c., are not those which distinguish the nebular spectrum. On the contrary, this spectrum is chiefly remarkable for a few brilliant lines, very...
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Report of the ... Meeting of the British Association for the ..., Volume 61

British Association for the Advancement of Science - 1892 - 1258 pages
...in 1871 by Sir William Thomson in his Presidential Address. The spectrum of the bright-line nebulae is certainly not such a spectrum as we should expect...magnesium, nickel, &c., are not those which distinguish the nebular spectrum. On the contrary, this spectrum is chiefly remarkable for a few brilliant lines, very...
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Congressional Serial Set

1892 - 790 pages
...in 1871 by Sir William Thomson in his presidential address. The spectrum of the bright-line nebula; is certainly not such a spectrum as we should expect...collisions of meteorites similar to those which have been analyzed in our laboratories. The strongest lines of the substances which in the case of such meteorites...
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Annual Report of the Board of Regents of the Smithsonian Institution

Smithsonian Institution. Board of Regents - 1893 - 816 pages
...in 1871 by Sir William Thomson in his presidential address. The spectrum of the bright-line nebulae is certainly not such a spectrum as we should expect...collisions of meteorites similar to those which have been analyzed in our laboratories. The strongest lines of the substances which in the case of such meteorites...
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Essays in Astronomy

1900 - 600 pages
...in 1871 by Sir William Thomson in his presidential address. The spectrum of the bright-line nebulae is certainly not such a spectrum as we should expect...collisions of meteorites similar to those which have been analyzed in our laboratories. The strongest lines of the substances which in the case of such meteorites...
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The Observatory, Volume 33

1910 - 526 pages
...the notice of the Association in 1871 by Sir William Thomson. The spectrum of the bright-line nebula; is certainly not such a spectrum as we should expect from the flushing by collisions of meteorites similar to those which have been analysed in our laboratories....
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Annual Report of the Board of Regents of the Smithsonian Institution

Smithsonian Institution. Board of Regents - 1893 - 784 pages
...in 1871 by Sir William Thomson in his presidential address. The spectrum of the bright-line nebula- is certainly not such a spectrum as we should expect...collisions of meteorites similar to those which have been analyzed in our laboratories. The strongest lines of the substances which in the case of such meteorites...
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Annual Report of the Board of Regents of the Smithsonian Institution

Smithsonian Institution. Board of Regents - 1893 - 862 pages
...expect from the flashing by collisions of meteorites similar to those which have been analyzed in onr laboratories. The strongest lines of the substances...show themselves, iron, sodium, magnesium, nickel, etc., are not those which distinguish the nebular spectrum. On the contrary, this spectrum is chiefly...
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