Publications

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/

  • Non-refereed
    Three MASTER OT's discovery
    The MASTER auto-detection system at Tunka (Baykal Lake) detected a new transient source at the position (R.A., Dec) = 17h 29m 00.07s , +75d 18m 42s.5, (J2000) with a typical uncertainty of 0.5" at 2011-05-12 18:24:47.725 (UT). The OT is seen at 2 images. There is no minor planet and any object brighter 21 mag in DSS at this place. The unfiltered (0
    Balanutsa, P. et al.

    Advertised on:

    5
    2011
    Bibcode
    2011ATel.3366....1B
    Citations
    1
  • Refereed
    The Swift/Fermi GRB 080928 from 1 eV to 150 keV
    We present the results of a comprehensive study of the gamma-ray burst 080928 and of its afterglow. GRB 080928 was a long burst detected by Swift/BAT and Fermi/GBM. It is one of the exceptional cases where optical emission had already been detected when the GRB itself was still radiating in the gamma-ray band. For nearly 100 s simultaneous optical
    Rossi, A. et al.

    Advertised on:

    5
    2011
    Bibcode
    2011A&A...529A.142R
    Citations
    56
  • Non-refereed
    The supergiant optical counterpart of ULX P13 in NGC 7793
    We have identified the optical counterpart of the ULX source P13 in the nearby spiral galaxy NGC 7793. The object is a V ˜ 20.5 mag star, ten times brighter than any other established counterpart of a ULX in nearby galaxies. Medium resolution optical spectroscopy carried out in 2008 and 2009 with the ESO-VLT reveals the presence of narrow high
    Motch, C. et al.

    Advertised on:

    5
    2011
    Bibcode
    2011AN....332..367M
    Citations
    56
  • Non-refereed
    The Solar Rotation and its Evolution During Cycle 23
    We present the most exhaustive and accurate inferences of the internal solar rotation rate and its evolution during solar cycle 23. A full solar cycle of MDI observations have been analyzed using our state of the art fitting methodology. Time series of various lengths have been fitted, from a single 4608-day long epoch (64 times 72 day or 12.6 yr)
    Korzennik, Sylvain G. et al.

    Advertised on:

    5
    2011
    Bibcode
    2011AAS...21822422K
    Citations
    0
  • Refereed
    The shortest period detached binary white dwarf system
    We identify SDSS J010657.39-100003.3 (hereafter J0106-1000) as the shortest period detached binary white dwarf (WD) system currently known. We targeted J0106-1000 as part of our radial velocity programme to search for companions around known extremely low-mass (ELM; ˜0.2 M&sun;) WDs using the 6.5-m Multiple Mirror Telescope. We detect peak-to-peak
    Kilic, Mukremin et al.

    Advertised on:

    5
    2011
    Bibcode
    2011MNRAS.413L.101K
    Citations
    47
  • Non-refereed
    The pathways of C: from AGB stars, to the Interstellar Medium, and finally into the protoplanetary disk
    The origin, and role of C in the formation of first solar system aggregates is described. Stellar grains evidence demonstrates that Asymptotic Giant Branch (AGB) stars were nearby to the solar nebula at the time of solar system formation. Such stars continue to burn H and He in shells that surround the C-O core. During their evolution, flashes
    Trigo-Rodriguez, J. M. et al.

    Advertised on:

    5
    2011
    Bibcode
    2011IAUS..280P.360T
    Citations
    0