IAUC 5131 available at Central Bureau for Astronomical Telegrams. IAUC 5131 available at Central Bureau for Astronomical Telegrams.
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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Supernova 1990E in NGC 1035Lopez, R. et al.111990
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Supernova 2004ao in UGC 10862
IAUC 8430 available at Central Bureau for Astronomical Telegrams.
Gomez, G. et al.Advertised on:
112004 -
Supernovae
IAUC 7745 available at Central Bureau for Astronomical Telegrams.
Barris, B. et al.Advertised on:
112001 -
Supernovae and Their Expanding Blast Waves during the Early Evolution of Galactic Globular Clusters
Our arguments deal with the early evolution of Galactic globular clusters and show why only a few of the supernovae (SNe) products were retained within globular clusters and only in the most massive cases (M ≥ 106 M⊙), while less massive clusters were not contaminated at all by SNe. Here, we show that SN blast waves evolving in a steep density
Tenorio-Tagle, G. et al.Advertised on:
112015 -
Supersonic Magnetic Upflows in Granular Cells Observed with SUNRISE/IMAX
Using the IMaX instrument on board the SUNRISE stratospheric balloon telescope, we have detected extremely shifted polarization signals around the Fe I 5250.217 Å spectral line within granules in the solar photosphere. We interpret the velocities associated with these events as corresponding to supersonic and magnetic upflows. In addition, they are
Borrero, J. M. et al.Advertised on:
112010 -
Suppression of cooling by strong magnetic fields in white dwarf stars
Isolated cool white dwarf stars more often have strong magnetic fields than young, hotter white dwarfs, which has been a puzzle because magnetic fields are expected to decay with time but a cool surface suggests that the star is old. In addition, some white dwarfs with strong fields vary in brightness as they rotate, which has been variously
Valyavin, G. et al.Advertised on:
112014