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The millimeter IRAM-30 m line survey toward IK TauExoplanetary Atmospheres-Chemistry, Formation Conditions, and HabitabilityReactivity of OH and CH3OH Between 22 and 64 K: Modelling the Gas Phase Production of CH3O in Barnard 1BHigh spatial resolution imaging of SO and H2CO in AB Auriga: The first SO image in a transitional diskA λ 3 mm and 1 mm line survey toward the yellow hypergiant IRC +10420: N-rich chemistry and IR flux variationsWarm water vapour in the sooty outflow from a luminous carbon star.Discovery of Time Variation of the Intensity of Molecular Lines in IRC+10216 in The Submillimeter and Far Infrared Domains.Probing non polar interstellar molecules through their protonated form: Detection of protonated cyanogen (NCCNH+).Discovery of SiCSi in IRC +10216: A missing link between gas and dust carriers of Si-C bonds.Molecular shells in IRC+10216: tracing the mass loss history(,.)The interstellar chemistry of H2C3O isomers.Revised spectroscopic parameters of SH(+) from ALMA and IRAM 30m observations.Discovery of interstellar ketenyl (HCCO), a surprisingly abundant radical.Si-bearing molecules toward IRC+10216: ALMA unveils the molecular envelope of CWLeoPhotodissociation of HCN and HNC isomers in the 7-10 eV energy range.The Photodissociation of HCN and HNC: Effects on the HNC/HCN Abundance Ratio in the Interstellar Medium.The Abundance of C2H4 in the Circumstellar Envelope of IRC+10216.Is the gas-phase OH+H2CO reaction a source of HCO in interstellar cold dark clouds? A kinetic, dynamic and modelling study.The peculiar distribution of CH_3_CN in IRC +10216 seen by ALMACarbon Chemistry in IRC+10216: Infrared Detection of Diacetylene.Discovery of Interstellar Isocyanogen (CNCN): Further Evidence that Dicyanopolyynes Are Abundant in SpaceAstronomical detection of C$\mathsf{_{4}H^-}$, the second interstellar anionHerschel/HIFI observation of highly excited rotational lines of HNC toward IRC +10 216On the physical structure of IRC +10216Spectroscopic parameters for silacyclopropynylidene, SiC2, from extensive astronomical observations toward CW Leo (IRC +10216) with the Herschel satelliteA high-resolution line survey of IRC +10216 withHerschel/HIFIDetection of anhydrous hydrochloric acid, HCl, in IRC +10216 with the HerschelSPIRE and PACS spectrometersPACS and SPIRE spectroscopy of the red supergiant VY CMaSilicon in the dust formation zone of IRC +10216Formation and Destruction of SiS in SpaceHints of the existence of C-rich massive evolved starsChemistry of dark clouds: databases, networks, and modelsStudy of CS, SiO, and SiS abundances in carbon star envelopes: Assessing their role as gas-phase precursors of dustThe Maser Emitting Structure and Time Variability of the SIS Lines J = 14 - 13 and 15 - 14 in IRC+10216
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description
forsker
@nb
researcher
@en
wetenschapper
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հետազոտող
@hy
name
M. Agúndez
@ast
M. Agúndez
@nl
Marcelino Agúndez
@en
Marcelino Agúndez
@es
Marcelino Agúndez
@nb
type
label
M. Agúndez
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M. Agúndez
@nl
Marcelino Agúndez
@en
Marcelino Agúndez
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Marcelino Agúndez
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altLabel
M. Agúndez
@en
prefLabel
M. Agúndez
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M. Agúndez
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Marcelino Agúndez
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Marcelino Agúndez
@es
Marcelino Agúndez
@nb
P106
P31
P496
0000-0003-3248-3564