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Complex organic molecules in the Galactic Centre: The N-bearing family
ArticleAbstract: We present an unbiased spectral line survey towards the Galactic Centre (GC) quiescent giant moleculPalabras claves:Galaxy: centre, ISM: abundances, ISM: clouds, ISM: moleculesAutores:Aladro R., J. Armijos-Abendaño, Jiménez-Serra I., Martín S., Martín-Pintado J., Requena-Torres M.A., Riquelme D., Rivilla V.M., Zeng S.Fuentes:scopusBroad-line region clouds orbiting an AGN sample
ArticleAbstract: We present a spectral and temporal analysis of XMM-Newton data from a sample of six galaxies (NGC 37Palabras claves:Galaxies: active, galaxies: nuclei, X-rays: galaxiesAutores:Ericson D. Lopez, J. Armijos-Abendaño, Jairo Armijos, Logan C.H.A., Mario LlerenaFuentes:googlescopus3-mm spectral line survey of two lines of sight towards two typical cloud complexes in the Galactic Centre
ArticleAbstract: We present the results of two Mopra 3-mm spectral line surveys of the lines of sight (LOS) towards tPalabras claves:Galaxy: centre, ISM: abundances, ISM: clouds, ISM: moleculesAutores:J. Armijos-Abendaño, Jairo Armijos, Martín S., Martín-Pintado J., Requena-Torres M.A., Rodríguez-Franco A.Fuentes:googlescopusA cloud-cloud collision in Sgr B2? 3D simulations meet SiO observations
Conference ObjectAbstract: We compare the properties of shocked gas in Sgr B2 with maps obtained from 3D simulations of a colliPalabras claves:Galaxy: centre, hydrodynamics, ISM: clouds, radio lines: ISMAutores:Dénes H., Helga Dénes, J. Armijos-Abendaño, Jairo Armijos, Wladimir E. Banda-BarragánFuentes:googlescopusAbundant Z-cyanomethanimine in the interstellar medium: Paving the way to the synthesis of adenine
ReviewAbstract: We report the first detection in the interstellar medium (ISM) of the Z-isomer of cyanomethanimine (Palabras claves:Galaxy: centre, ISM: abundances, ISM: clouds, ISM: moleculesAutores:Aladro R., J. Armijos-Abendaño, Jiménez-Serra I., Martín S., Martín-Pintado J., Requena-Torres M.A., Riquelme D., Rivilla V.M., Zeng S.Fuentes:scopusDust deficiency in the interacting galaxy NGC 3077
ArticleAbstract: Using 70 μm observations taken with the PACS instrument of the Herschel space telescope, the dust coPalabras claves:Dust mass, Dust-to-gas ratio, Spiral galaxiesAutores:Ericson D. Lopez, Franklin Aldás, J. Armijos-Abendaño, Logan C.H.A., Mario LlerenaFuentes:googlescopusLambda = 3 mm line survey of nearby active galaxies
ArticleAbstract: Aims. We aim to better understand the imprints that the nuclear activity in galaxies leaves in the mPalabras claves:Galaxies: abundances, Galaxies: active, galaxies: ISM, galaxies: nuclei, ISM: molecules, radio lines: ISMAutores:Aladro R., Henkel C., J. Armijos-Abendaño, Kramer C., Lefevre C., Martín S., Martín-Pintado J., Mauersberger R., Requena-Torres M.A., Riquelme D., Weiß A.Fuentes:scopusHerschel water maps towards the vicinity of the black hole Sgr A∗
ArticleAbstract: Aims. We study the spatial distribution and kinematics of water emission in a ~8 × 8 pc2 region of tPalabras claves:Galaxy: nucleus, ISM: abundances, ISM: moleculesAutores:González-Alfonso E., Güsten R., Harris A.I., Israel F.P., J. Armijos-Abendaño, Kramer C., Martín-Pintado J., Requena-Torres M.A., Stutzki J., Van Der Werf P., Weiß A.Fuentes:scopusOn the Effects of UV Photons/X-Rays on the Chemistry of the Sgr B2 Cloud
ArticleAbstract: The lines of HOC+, HCO, and CO+ are considered good tracers of photon-dominated regions (PDRs) and XPalabras claves:Autores:Ericson D. Lopez, Franklin Aldás, Harada N., J. Armijos-Abendaño, Mario Llerena, Martín S., Martín-Pintado J., Requena-Torres M.A., Riquelme D., Rivilla V.M.Fuentes:googlescopusPhosphorus-bearing molecules in the Galactic Center
ArticleAbstract: Phosphorus (P) is one of the essential elements for life due to its central role in bio- chemical prPalabras claves:Galaxy: centre, ISM: abundances, ISM: clouds, ISM: moleculesAutores:Aladro R., Beltrán M.T., Fontani F., J. Armijos-Abendaño, Jairo Armijos, Jiménez-Serra I., Martín S., Martín-Pintado J., Quénard D., Requena-Torres M.A., Riquelme D., Rivilla V.M., Viti S., Zeng S.Fuentes:googlescopus