Two Apparent Novae in M81: M81N 2010-06a and M81N 2010-06b
CBET 2332 available at Central Bureau for Astronomical Telegrams.
Hornoch, K. et al.
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2010
This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..
It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/
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Two Apparent Novae in M81: M81N 2010-06a and M81N 2010-06bCBET 2332 available at Central Bureau for Astronomical Telegrams.Garnavich, P. et al.
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62010 -
Two Apparent Novae in M81: M81N 2010-06a and M81N 2010-06bCBET 2332 available at Central Bureau for Astronomical Telegrams.Garnavich, P. et al.
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62010 -
Transverse Oscillations of a Multi-stranded LoopWe investigate the transverse oscillations of a line-tied multi-stranded coronal loop composed of several parallel cylindrical strands. First, the collective fast normal modes of the loop are found with the T-matrix theory. There is a huge quantity of normal modes with very different frequencies and a complex structure of the associated magneticLuna, M. et al.
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62010 -
Time-Resolved Rotational Energy Transfer and Spectral Line Broadening in Acetylene. a High Resolution Raman Study.The quasi-cw stimulated Raman technique is a powerful tool for the determination of collisional broadening and line-mixing parameters, which bear a very direct relationship with the rotational energy transfer rate constants matrix at the state-to-state level. Indeed, the broadening coefficients and the analysis of line-mixing profiles, frequentlyDomenech, J. L. et al.
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62010 -
The VLT-FLAMES Survey of Massive StarsThe VLT-FLAMES Survey of Massive Stars in the Galaxy, the Large and Small Magellanic Clouds was an ESO Large Program (P.I. S. Smartt) aimed at understanding rotational mixing and stellar mass loss in environments of differing metallicity (Z). The overarching goal is to better understand massive star evolution.Lennon, D. J. et al.
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62010