Výsledky vyhledávání - "M. Chavez-Dagostino"

Interstellar Complex Organic Molecules in SiO-traced massive outflows

Autor: O. S. Rojas-García, A. I. Gómez-Ruiz, A. Palau, M. T. Orozco-Aguilera, M. Chavez Dagostino, S. E. Kurtz

The interstellar medium contains dust and gas, in which at high densities and cold conditions molecules can proliferate. Interstellar Complex Organic Molecules (iCOMs) are C-bearing species that contain at least six atoms. As they are detected in you

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::265f47519b4f416285e91546c69a10a3

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LMT/AzTEC observations of Vega

Autor: J P Marshall, M Chavez-Dagostino, D Sanchez-Arguelles, L Matrà, C del Burgo, F Kemper, E Bertone, W R F Dent, O Vega, G Wilson, A Gómez-Ruiz, A Montaña

Publikováno v: Digital.CSIC. Repositorio Institucional del CSIC
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Vega is the prototypical debris disc system. Its architecture has been extensively studied at optical to millimetre wavelengths, revealing a near face-on, broad, and smooth disc with multiple distinct components. Recent millimetre-wavelength observat

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b6fcb2b09277dbd27a419b150522680e
http://hdl.handle.net/10261/279889

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Wandering near the red edge: photometric observations of three cool ZZ Ceti stars

Autor: D. I. Jenei, M. Chavez-Dagostino, M. Paparó, Zs. Bognár, E. Verebélyi, H. Ollé, Emese Plachy, Péter Pápics, Ádám Sódor, Michael H. Montgomery, Cs. Kalup, Emanuele Bertone, Á. Győrffy, László Molnár

Publikováno v: Monthly Notices of the Royal Astronomical Society. 482:4018-4031

We summarize our findings on three cool ZZ Ceti type pulsating white dwarfs. We determined eight independent modes in HS 0733+4119, of which seven are new findings. For GD 154, we detected two new eigenmodes, and the recurrence of the pulsational beh

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::220aef21108d294f1a50b7dfbf6240f2
https://doi.org/10.1093/mnras/sty2884

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Early science with the Large Millimeter Telescope: molecules in the extreme outflow of a protoplanetary nebula

Autor: Lizette Guzman-Ramirez, Raghvendra Sahai, Alfredo Montaña, A Luna, Arturo I. Gómez-Ruiz, David H. Hughes, Albert A. Zijlstra, F. P. Schloerb, Gopal Narayanan, M. Chavez-Dagostino, David Sánchez-Arguelles, E. O. Serrano, Mónica Rodríguez, M. S. Yun

Publikováno v: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (ISSN 0035-8711), 467(1), L61-L65
Gómez-Ruiz, A I, Guzman-Ramirez, L, Serrano, E O, Sanchez-Argüelles, D, Luna, A, Schloerb, F P, Narayanan, G, Yun, M S, Sahai, R, Zijlstra, A, Chavez-Dagostino, M, Montaña, A, Hughes, D H & Rodríguez, M 2017, ' Early Science with the Large Millimetre Telescope : Molecules in the Extreme Outflow of a proto-Planetary Nebula ', Monthly Notices of the Royal Astronomical Society, vol. 467, no. 1, pp. L61-L65 . https://doi.org/10.1093/mnrasl/slw259

Extremely high velocity emission likely related to jets is known to occur in some proto-Planetary Nebulae. However, the molecular complexity of this kinematic component is largely unknown. We observed the known extreme outflow from the proto-Planetar

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::247a0f1b9336c7180ed40e046a1a8147
https://doi.org/10.1093/mnrasl/slw259

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