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Results 1 to 25 of 1018

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The unusual nickel/iron abundance ratio in the Crab nebula filamentsHENRY, R. B. C.The Astrophysical journal. 1984, Vol 281, Num 2, pp 644-649, issn 0004-637X, 1Article

Theoretical investigation of the interstellar CH3NC/CH3CN ratioDEFREES, D. J; MCLEAN, A. D; HERBST, E et al.The Astrophysical journal. 1985, Vol 293, Num 1, pp 236-242, issn 0004-637XArticle

Galactic chronology of thorium/neodymium. RepliesFOWLER, W. A; BUTCHER, H; NOERDLINGER, P. D et al.Nature (London). 1987, Vol 330, Num 6150, pp 703-704, issn 0028-0836Article

Sub-iron to iron nuclei in low-energy (50-200 MeV nucl-1) cosmic rays as observed in the skylab experimentDURGAPRASAD, N; BISWAS, S.Astrophysics and space science. 1988, Vol 149, Num 1, pp 163-170, issn 0004-640XArticle

The interstellar N/O abundance ratio : Evidence for local infall?'KNAUTH, David C; MEYER, David M; LAUROESCH, James T et al.The Astrophysical journal. 2006, Vol 647, Num 2, issn 0004-637X, L115-L118, 2Article

A reanalysis of the HCO+/HOC+ abundance ratio in dense interstellar cloudsJARROLD, M. F; BOWERS, M. T; DEFREES, D. J et al.The Astrophysical journal. 1986, Vol 303, Num 1, pp 392-400, issn 0004-637X, 1Article

OXYGEN-TO-NEON ABUNDANCE RATIO IN THE SOLAR CORONA.ACTON LW; CATURA RC; JOKI EG et al.1975; ASTROPHYS. J.; U.S.A.; DA. 1975; VOL. 195; NO 2 PART. 2; PP. L93-L95; BIBL. 11 REF.Article

Why did Comet 17P/Holmes burst out? : Nucleus splitting or delayed sublimation?ALTENHOFF, W. J; KREYSA, E; MENTEN, K. M et al.Astronomy and astrophysics (Berlin. Print). 2009, Vol 495, Num 3, pp 975-978, issn 0004-6361, 4 p.Article

Anomalous nitrogen isotope ratio in cometsARPIGNY, Claude; JEHIN, Emmanuël; MANFROID, Jean et al.Science (Washington, D.C.). 2003, Vol 301, Num 5639, pp 1522-1524, issn 0036-8075, 3 p.Article

The deuterium-to-hydrogen abundance ratio toward the QSO SDSS J155810.16-003120.0O'MEARA, John M; BURLES, Scott; PROCHASKA, Jason X et al.The Astrophysical journal. 2006, Vol 649, Num 2, issn 0004-637X, L61-L65, 2Article

On the measurement of elemental abundance ratios in inner Galaxy H II regionsSIMPSON, Janet P; RUBIN, Robert H; COLGAN, Sean W. J et al.The Astrophysical journal. 2004, Vol 611, Num 1, pp 338-352, issn 0004-637X, 15 p., 1Article

Evidence for anomalous cosmic-ray hydrogenCHRISTIAN, E. R; CUMMINGS, A. C; STONE, E. C et al.The Astrophysical journal. 1988, Vol 334, Num 2, pp L77-L80, issn 0004-637XArticle

Solar wind carbon, nitrogen and oxygen abundances measured in the earth's magnetosheath with AMPTE/CCEGLOECKLER, G; IPAVICH, F. M; HAMILTON, D. C et al.Geophysical research letters. 1986, Vol 13, Num 8, pp 793-796, issn 0094-8276Article

Simple leaky box model for cosmic-ray propagation, models for production of antiprotons at ultrahigh energies and the estimations of the p/p ratiosBHATTACHARYYA, S; PRATIBHA PAL.Nuovo cimento della società italiana di fisica. C. 1986, Vol 9, Num 5, pp 961-983, issn 0390-5551Article

An XMM-Newton study of the RGH 80 galaxy groupXUE, Y.-J; BÖHRINGER, H; MATSUSHITA, K et al.Astronomy and astrophysics (Berlin. Print). 2004, Vol 420, Num 3, pp 833-845, issn 0004-6361, 13 p.Article

Detection of formaldehyde toward the extreme carbon star IRC +10216SAAVIK FORD, K. E; NEUFELD, David A; SCHILKE, Peter et al.The Astrophysical journal. 2004, Vol 614, Num 2, pp 990-1006, issn 0004-637X, 17 p., 1Article

Sublimation from icy jets as a probe of the interstellar volatile content of cometsBLAKE, G. A; QI, C; HOGERHEIJDE, M. R et al.Nature (London). 1999, Vol 398, Num 6724, pp 213-216, issn 0028-0836Article

CALCIUM-TO-ARGON AND NICKEL-TO-ARGON ABUNDANCE RATIOS AS TRACERS OF THE SOURCE REGION OF POSTFLARE LOOP SYSTEM MATERIALWIDING, K. G; FELDMAN, U.The Astrophysical journal. 2008, Vol 675, Num 1, pp 863-867, issn 0004-637X, 5 p., 1Article

Les comètes, source possibles de matériaux organiques terrestres = Comets, possibles sources of terrestrials organics materialsLEVASSEUR-REGOURD, A.-C.L' Astronomie (1911). 1989, Num 12, pp 495-497, issn 0004-6302, 3 p.Article

Para/ortho abundance ratio of molecular hydrogen in NGC 2023TAKAYANAGI, K; SAKIMOTO, K; ONDA, K et al.The Astrophysical journal. 1987, Vol 318, Num 2, pp L81-L84, issn 0004-637X, 2Article

Teneur relative en ions lourds dans la zone intérieure des ceintures de rayonnementPANASYUK, M. I.Kosmičeskie issledovaniâ. 1985, Vol 23, Num 5, pp 754-765, issn 0023-4206Article

Measurement of the formaldehyde ortho to para ratio in three molecular cloudsKAHANE, C; FRERKING, M. A; LANGER, W. D et al.Astronomy and astrophysics (Berlin. Print). 1984, Vol 137, Num 2, pp 211-222, issn 0004-6361Article

Minor ion composition in the polar ionosphereYAU, A. W; WHALEN, B. A; SAGAWA, E et al.Geophysical research letters. 1991, Vol 18, Num 2, pp 345-348, issn 0094-8276, 4 p.Article

Some comments on the asymptotic limit of antiproton-proton flux ratio at the top of the atmosphereALLKOFER, O. C; BHATTACHARYYA, D. P.Astrophysics and space science. 1987, Vol 132, Num 1, pp 141-146, issn 0004-640XArticle

Molecular abundance ratios as a tracer of accelerated collapse in regions of high-mass star formationLINTOTT, C. J; VITI, S; RAWLINGS, J. M. C et al.The Astrophysical journal. 2005, Vol 620, Num 2, pp 795-799, issn 0004-637X, 5 p., 1Article

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