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/

  • 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.

    Advertised on:

    1
    2015
    Citations
    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.

    Advertised on:

    1
    2015
    Citations
    27
  • 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.

    Advertised on:

    1
    2015
    Citations
    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.

    Advertised on:

    1
    2015
    Citations
    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.

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    1
    2015
    Citations
    0
  • 5 months of AMOS on the Canary Islands
    We present the technology, its installation and the first results from the AMOS meteor system on the Canary Islands. Since March 15 2015, a pair of AMOS automatic all-sky cameras (at Observatory Teide (Tenerife) and Roque de los Muchachos (La Palma) of the Astronomical Institute of Canary Islands) has been observing regularly to record meteors on
    Tóth, J. et al.

    Advertised on:

    1
    2015
    Citations
    6