No Nova in M32 (M32N 2010-07a)
CBET 2398 available at Central Bureau for Astronomical Telegrams.
Hornoch, K. et al.
Advertised on:
8
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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Non-LTE Determination of the Silicon Abundance Using a Three-dimensional Hydrodynamical Model of the Solar PhotosphereConfrontations of spectroscopic observations with local thermodynamic equilibrium (LTE) spectral syntheses in a three-dimensional (3D) hydrodynamical model of the solar photosphere led to a downward revision of the photospheric and meteoritic silicon abundances. Here we derive the photospheric silicon abundance taking into account non-LTE (NLTE)Shchukina, N. et al.
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82012 -
Non-LTE Model Atmospheres for Late-Type Stars. I. A Collection of Data for Light Neutral and Singly Ionized AtomsWith the goal of producing a reliable set of model atoms and singly ionized ions for use in building NLTE model atmospheres, we have combined measured energy levels, critically compiled line transition probabilities, and resonance-averaged calculations of photoionization cross sections. A majority of the elements from Li to Ca are consideredAllende Prieto, Carlos et al.
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82003 -
Nova Vulpeculae 1984IAUC 3977 available at Central Bureau for Astronomical Telegrams. IAUC 3977 available at Central Bureau for Astronomical Telegrams.Maley, P. et al.
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81984 -
Novel dispersive elements for LIRISNew dispersive elements providing relative high resolution (R=2200) have been recently incorporated in the near infrared spectrograph LIRIS. These elements are founded on a rather novel design based on a diffractive pattern engraved in fused silica, which is placed between two prisms. These new components are pushing forward the scientificFragoso-López, Ana B. et al.
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82008 -
Nuclear Activity and Massive Star Formation in the Low-Luminosity Active Galactic Nucleus NGC 4303: Chandra X-Ray ObservationsWe present evidence of the coexistence of either an AGN or an ultraluminous X-ray source, together with a young superstellar cluster, in the central 3 pc of NGC 4303. The galaxy contains a low-luminosity AGN and hosts a number of starburst regions in a circumnuclear spiral, as well as in the nucleus itself. A high spatial resolution Chandra imageJiménez-Bailón, E. et al.
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82003