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/

  • Planetary nebulae hosting accreting white dwarfs: a possible solution for the mysterious cut-off of planetary nebula luminosity function?
    Many binary companions to the central stars of planetary nebulae (PNe) are found to be inflated, perhaps indicating that accretion onto the central star might occur during the planetary nebula (PN) phase. The discovery of a handful of nova eruptions and supersoft X-ray sources inside PNe supports this hypothesis. In this paper, we investigate the
    Souropanis, D. et al.

    Advertised on:

    5
    2023
    Citations
    3
  • The AGNIFS survey: spatially resolved observations of hot molecular and ionized outflows in nearby active galaxies
    We present the hot molecular and warm ionized gas kinematics for 33 nearby (0.001 ≲ z ≲ 0.056) X-ray selected active galaxies using the H$_2\, 2.1218\, \mu$m and Br γ emission lines observed in the K band with the Gemini near-infrared integral field spectrograph. The observations cover the inner 0.04-2 kpc of each active galactic nucleus at spatial
    Riffel, R. A. et al.

    Advertised on:

    5
    2023
    Citations
    19
  • IONISED GAS FLOWS IN THE ORION NEBULA: PROPERTIES AND ENVIRONMENTAL DEPENDENCES
    This PhD thesis is dedicated to the analysis of Herbig-Haro objects (HHs) in the central region of the Orion Nebula and their impact on the surrounding ionised gas. HHs are collimated gas jets ejected from protostars. Although their physical properties and excitation mechanism have been extensively studied in neutral gas clouds, those HHs immersed
    José Eduardo Méndez Delgado

    Advertised on:

    9
    2022
  • INSTRUMENTATION FOR THE TENERIFE MICROWAVE SPECTROMETER
    El interés por desentrañar la historia térmica del Universo infante, codificada en la distribución espectral del fondo cósmico de microondas (FCM), ha sido durante mucho tiempo una fuerza impulsora en la comunidad científica. Recientemente se han propuesto nuevas misiones espaciales para detectar distorsiones espectrales a alta frecuencia
    Paz Alonso Árias

    Advertised on:

    10
    2022
  • THREE-DIMENSIONAL SIMULATIONS OF THE GENERATION AND TRANSFER OF SPECTRAL LINE POLARIZATION IN THE SOLAR CHROMOSPHERE
    El campo magnético es la causa principal de los espectaculares fenómenos que observamos en las capas externas de la atmósfera solar (la cromosfera, la región de transición y la corona), tales como el calentamiento del plasma hasta cientos de miles y millones de grados, o las eyecciones de masa coronal que pueden perturbar seriamente la magnetosfera
    Jaume Jaume Bestard

    Advertised on:

    12
    2022
  • COSMOLOGY FROM QUASAR MICROLENSING
    La cosmología actual se encuentra en constante cambio debido a los nuevos descubrimientos en una gran variedad de campos de la física y astrofísica modernas. Parte de estos hallazgos se deben al efecto lente gravitatoria que, entre otras cosas, proporciona información detallada sobre la composición de las galaxias y de sus velocidades peculiares
    Ana Esteban Gutiérrez

    Advertised on:

    7
    2022