Publicaciones

Esta sección ofrece el acceso a la base de datos de Publicaciones que recopila los artículos del IAC publicados en revistas científicas. Por favor, pulsa la flecha del menú para ver todas las opciones de búsqueda y de ordenación de resultados; autor, revista, año, etc..

Además ofrece acceso al  repositorio de preprints del IAC: https://research.iac.es/preprints/l

  • Analyzing Star Formation Properties in Dusty Early Universe Galaxies Using Gravitational Lensing
    Strong gravitational lensing has recently become one of the most important tools for studying star formation properties in extremely high redshift galaxies. Dust-obscured star-forming galaxies found at far-infrared/sub-millimeter wavelengths are important in the assembly of stellar mass and the evolution of massive galaxies. We present
    Bradli, J. C. et al.

    Fecha de publicación:

    1
    2015
    Número de citas
    0
  • Analysis of Co-spatial UV-Optical STIS Spectra of Planetary Nebulae From HST Cycle 19 GO 12600
    We present an analysis of five spatially resolved planetary nebulae (PNe), NGC 5315, NGC 5882, NGC 7662, IC 2165, and IC 3568, from observations in the Cycle 19 program GO 12600 using HST STIS. Details of the observations and data are presented in the poster by Dufour et al. in this session. These five observations cover the wavelength range 1150
    Miller, T. R. et al.

    Fecha de publicación:

    1
    2015
    Número de citas
    0
  • A search for diffuse bands in fullerene planetary nebulae: evidence of diffuse circumstellar bands
    Large fullerenes and fullerene-based molecules have been proposed as carriers of diffuse interstellar bands (DIBs). The recent detection of the most common fullerenes (C60 and C70) around some planetary nebulae (PNe) now enable us to study the DIBs towards fullerene-rich space environments. We search DIBs in the optical spectra towards three
    Díaz-Luis, J. J. et al.

    Fecha de publicación:

    1
    2015
    Número de citas
    26
  • A Puzzling Li-rich Red Giant in the APOGEE Field
    We report on a spectroscopic study of the unusual Li-rich red giant (RG) recently discovered in NGC 6819. This star was observed by the Apache Point Observatory Galactic Evolution Experiment (APOGEE) survey as part of the survey's calibration cluster sample. We use the high-resolution, near-infrared APOGEE spectrum to address its questionable
    Carlberg, J. K. et al.

    Fecha de publicación:

    1
    2015
    Número de citas
    0
  • A Pipeline for the Analysis of APOGEE Spectra Based on Equivalent Widths
    The Apache Point Galactic Evolution Experiment (APOGEE) forms part of the third Sloan Digital Sky Survey and has obtained high resolution, high signal-to-noise infrared spectra for ~1.3 x 105 stars across the galactic bulge, disc and halo. From these, stellar parameters are derived together with abundances for various elements using the APOGEE
    Arfon Williams, R. et al.

    Fecha de publicación:

    1
    2015
    Número de citas
    0
  • A Detailed Characterization of the Milky Way Bulge with APOGEE
    An important part of the history of the Milky Way is encoded in the dynamics and chemistry of the inner Galaxy, which contains about 30% of its mass. It is only in the last few years that a composite picture of the bulge has begun to emerge: recent evidence points towards a population made of multiple components. The origin of the bulge appears to
    García Pérez, A. E. et al.

    Fecha de publicación:

    1
    2015
    Número de citas
    0