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| Query : 2012ApJ...754L..41L |
2012ApJ...754L..41L - Astrophys. J., 754, L41 (2012/August-1)
Laboratory analysis of presolar silicate stardust from a nova.
LEITNER J., KODOLANYI J., HOPPE P. and FLOSS C.
Abstract (from CDS):
Auger electron spectroscopic analyses identify O, Mg, Si, and Fe as the grain's major constituents. Its (Mg+Fe)/Si atomic ratios are lower than that of olivine and correspond on average to Fe-Mg-pyroxene. A complex texture and heterogeneous major element distribution within the grain attest to condensation under non-equilibrium conditions, which is consistent with the proposed nova origin.
Abstract Copyright: ∼
Journal keyword(s): astrochemistry - circumstellar matter - novae, cataclysmic variables - nuclear reactions, nucleosynthesis, abundances - stars: winds, outflows
Simbad objects: 1
| Number of rows : 1 |
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Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
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1850 - 2026 |
#notes |
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| 1 | SN 2011fe | SN* | 14 03 05.711 | +54 16 25.22 | 10.12 | 10.06 | SNIa-norm | 747 | 1 |
| Query : 2012ApJ...754L..41L |
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| SN 2011fe | PSN J14030581+5416254 | PTF 11kly |
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References (747 between 1850 and 2026) (Total 747)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system). |
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