Possible Nova in M31: M31N 2010-10b
CBET 2487 available at Central Bureau for Astronomical Telegrams.
Corral-Santana, J. et al.
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10
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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Possible nova in M31: M31N 2010-10b.CBET 2487 available at Central Bureau for Astronomical Telegrams.Hornoch, K. et al.
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102010 -
Post-AGB stars with hot circumstellar dust: binarity of the low-amplitude pulsatorsContext: The influence of binarity on the late stages of stellar evolution remains an open issue. Aims: While the first binary post-AGB stars were serendipitously discovered, the distinct characteristics of their spectral energy distribution (SED) allowed us to launch a more systematic search for binaries. We selected post-AGB objects, whichvan Winckel, H. et al.
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102009 -
Power Spectra of Velocities and Magnetic Fields on the Solar Surface and their Dependence on the Unsigned Magnetic Flux DensityWe have performed power spectral analysis of surface temperatures, velocities, and magnetic fields, using spectropolarimetric data taken with the Hinode Solar Optical Telescope. When we make power spectra in a field of view covering the supergranular scale, kinetic and thermal power spectra have a prominent peak at the granular scale while theKatsukawa, Y. et al.
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102012 -
Precise radial velocities of giant stars. IX. HD 59686 Ab: a massive circumstellar planet orbiting a giant star in a 13.6 au eccentric binary systemContext. For over 12 yr, we have carried out a precise radial velocity (RV) survey of a sample of 373 G- and K-giant stars using the Hamilton Échelle Spectrograph at the Lick Observatory. There are, among others, a number of multiple planetary systems in our sample as well as several planetary candidates in stellar binaries. Aims: We aim atOrtiz, M. et al.
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102016 -
Precise surface gravities of δ Scuti stars from asteroseismologyThe work reported here demonstrates that it is possible to accurately determine surface gravities of δ Scuti (δ Sct) stars using the frequency content from high-precision photometry and a measurement of the parallax. Using a sample of 10 eclipsing binary systems with a δ Sct component and the unique δ Sct star discovered with a transiting planetGarcía Hernández, A. et al.
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102017