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/

  • Refereed
    9+ frequencies for V534 Tauri, a δ Scuti variable in the Pleiades. Results of the STEPHI IX campaign
    New observations of V534 Tau were performed during the STEPHI IX campaign in November 1998. An overall run of 285 h of data has been collected from three sites over a period of 23 days. Period analysis reveals a rich oscillation spectrum with nine frequencies above the 99% confidence level. This oscillation spectrum spans a large range of
    Li, Z.-P. et al.

    Advertised on:

    6
    2004
    Bibcode
    2004A&A...420..283L
    Citations
    12
  • Refereed
    The X-ray binary X2127+119 in M15: evidence for a very low mass, stripped-giant companion
    We present integral field spectroscopy of X2127+119, the luminous X-ray binary in the globular cluster M15, obtained with INTEGRAL/WYFFOS on the William Herschel Telescope. We find that tomograms of HeIIλ4686 line profiles appear to be incompatible with the previously assumed view of X2127+119, in which the binary consists of a 1.4-Msolar neutron
    van Zyl, L. et al.

    Advertised on:

    5
    2004
    Bibcode
    2004MNRAS.350..649V
    Citations
    17
  • Refereed
    The Quest for Microwave Foreground X
    The Wilkinson Microwave Anisotropy Probe (WMAP) team has produced a foreground map that can account for most of the low-frequency Galactic microwave emission in the WMAP maps, tentatively interpreting it as synchrotron emission. Finkbeiner and collaborators have challenged these conclusions, arguing that the WMAP team's ``synchrotron'' template is
    de Oliveira-Costa, Angélica et al.

    Advertised on:

    5
    2004
    Bibcode
    2004ApJ...606L..89D
    Citations
    95
  • Non-refereed
    The Photodetector Array Camera and Spectrometer (PACS) for the Herschel Space Observatory
    The Photodetector Array Camera and Spectrometer (PACS) is one of the three science instruments for ESA's far infrared and submillimetre observatory Herschel. It employs two Ge:Ga photoconductor arrays (stressed and unstressed) with 16 × 25 pixels, each, and two filled Si bolometer arrays with 16 × 32 and 32 × 64 pixels, respectively, to perform
    Poglitsch, A. et al.

    Advertised on:

    5
    2004
    Bibcode
    2004AAS...204.9302P
    Citations
    0
  • Non-refereed
    The periods of the β Cephei star κ Scorpii as observed by WIRE
    The β Cephei star κ Scorpii is known to be multiperiodic from old photometric observations. A main period of 4.8 hr was detected, and from a beat period of about 7 d a secondary period of 4.9 hr was calculated. These periods were also found in recently analyzed line profile data. In two short data sets (separated by 152 d) obtained by the star
    Cuypers, J. et al.

    Advertised on:

    5
    2004
    Bibcode
    2004ASPC..310..251C
    Citations
    3
  • Refereed
    The non-radially pulsating primary of the cataclysmic variable GW Librae
    The dwarf nova GW Librae (GW Lib) is the first cataclysmic variable (CV) discovered to have a primary in a white dwarf instability strip, making it the first multimode, non-radially pulsating star known to be accreting. The primaries of CVs, embedded in hot, bright accretion discs, are difficult to study directly. Applying the techniques of
    van Zyl, L. et al.

    Advertised on:

    5
    2004
    Bibcode
    2004MNRAS.350..307V
    Citations
    78