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
    Indirect evidence for an active radio pulsar in SAX J1808.4-3658 during quiescence

    Millisecond radio pulsars are neutron stars that have been spun-up by the transfer of angular momentum during the low-mass X-ray binary phase. The transition from an accretion-powered to a rotation-powered pulsar takes place on evolutionary timescales at the end of the accretion process, however it may also occur sporadically in systems undergoing

    Campana, S. et al.

    Advertised on:

    10
    2005
    Bibcode
    2005AIPC..797...81C
    Citations
    2
  • Refereed
    Indirect Evidence of an Active Radio Pulsar in the Quiescent State of the Transient Millisecond Pulsar SAX J1808.4-3658

    Millisecond radio pulsars are neutron stars that have been spun up by the transfer of angular momentum during the low-mass X-ray binary phase. The transition from an accretion-powered pulsar to a rotation-powered pulsar takes place on evolutionary timescales at the end of the accretion process; however, it may also occur sporadically in systems

    Campana, Sergio et al.

    Advertised on:

    10
    2004
    Bibcode
    2004ApJ...614L..49C
    Citations
    68
  • Refereed
    Infrared flux excesses from hot subdwarfs. II. 72 more objects

    In our search, started in February, 1994, for JHK excess fluxes among the hot subdwarf population as an indicator for the presence of binary companions, results for 72 more hot objects (=63 hot subdwarfs + 1 Horizontal Branch B star + 7 white dwarfs + 1 non-subdwarf object) observed with the Carlos Sanchez CVF IR photometer (in June and October

    Ulla, A. et al.

    Advertised on:

    10
    1998
    Bibcode
    1998A&AS..132....1U
    Citations
    52
  • Refereed
    Infrared High-resolution Integrated Light Spectral Analyses of M31 Globular Clusters from APOGEE

    Chemical abundances are presented for 25 M31 globular clusters (GCs), based on moderately high resolution (R = 22,500) H-band integrated light (IL) spectra from the Apache Point Observatory Galactic Evolution Experiment (APOGEE). Infrared (IR) spectra offer lines from new elements, lines of different strengths, and lines at higher excitation

    Sakari, C. M. et al.

    Advertised on:

    10
    2016
    Bibcode
    2016ApJ...829..116S
    Citations
    33