Zobrazeno 1 - 10
of 148
pro vyhledávání: '"Dómenech, Rafael"'
Autor:
Martin-Domenech, Rafael, Öberg, Karin I., Caro, Guillermo M. Muñoz, de Lucas, Héctor Carrascosa, Fuente, Asunción, Rajappan, Mahesh
Understanding the formation of carbonyl sulfide (OCS) in interstellar ices is key to constrain the sulfur chemistry in the interstellar medium (ISM), since it is the only ice S-bearing molecule securely detected thus far. Two general pathways for OCS
Externí odkaz:
http://arxiv.org/abs/2410.07736
Ice chemistry in the dense, cold interstellar medium (ISM) is probably responsible for the formation of interstellar complex organic molecules (COMs). Recent laboratory experiments performed at T=4 K have shown that irradiation of CO:N2 ice samples a
Externí odkaz:
http://arxiv.org/abs/2401.04024
Autor:
Rodríguez-Baras, Marina, Esplugues, Gisela, Fuente, Asunción, Spezzano, Silvia, Caselli, Paola, Loison, Jean-Christophe, Roueff, Evelyne, Navarro-Almaida, David, Bachiller, Rafael, Martín-Doménech, Rafael, Jiménez-Serra, Izaskun, Beitia-Antero, Leire, Gal, Romane Le
H2S is thought to be the main sulphur reservoir in the ice, being therefore a key molecule to understand sulphur chemistry in the star formation process and to solve the missing sulphur problem. The H2S deuterium fraction can be used to constrain its
Externí odkaz:
http://arxiv.org/abs/2309.00318
Autor:
Maksyutenko, Pavlo, Martin-Domenech, Rafael, Piacentino, Elettra, Oberg, Karin I., Rajappan, Mahesh
Benzonitrile (c-C6H5CN) has been recently detected in cold and dense regions of the interstellar medium (ISM), where it has been used as a signpost of a rich aromatic organic chemistry that might lead to the production of polycyclic aromatic hydrocar
Externí odkaz:
http://arxiv.org/abs/2210.03827
Autor:
Martin-Domenech, Rafael, Bergner, Jennifer B., Oberg, Karin I., Carpenter, John, Law, Charles J., Huang, Jane, Jorgensen, Jes K., Schwarz, Kamber, Wilner, David J.
We report the detection of more than 120 emission lines corresponding to 8 complex organic molecules (CH3OH, CH3CH2OH, CH3OCH3, CH3OCHO, CH3COCH3, NH2CHO, CH2DCN, and CH3CH2CN) and 3 isotopologues (CH2DOH, 13CH3CN, and CH3C15N) toward the western com
Externí odkaz:
http://arxiv.org/abs/2109.11512
Interstellar ice mantles on the surfaces of dust grains are thought to have a bi-layered structure, with a H2O-rich polar layer, covered by a CO-rich apolar layer that probably harbors H2 and other volatiles such as N2. In this work, we explore the c
Externí odkaz:
http://arxiv.org/abs/2009.01335
Complex organic molecules (COMs) can be produced by energetic processing of interstellar ice mantles accreted on top of dust grains. Two COMs with proposed energetic ice formation pathways are formamide and acetaldehyde. Both have been detected in So
Externí odkaz:
http://arxiv.org/abs/2004.01151
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Autor:
Bergner, Jennifer B., Martin-Domenech, Rafael, Oberg, Karin I., Jorgensen, Jes K., de la Villarmois, Elizabeth Artur, Brinch, Christian
We present ALMA observations of organic molecules towards five low-mass Class 0/I protostellar disk candidates in the Serpens cluster. Three sources (Ser-emb 1, Ser-emb 8, and Ser-emb 17) present emission of CH3OH as well as CH3OCH3, CH3OCHO, and CH2
Externí odkaz:
http://arxiv.org/abs/1907.07791
Autor:
Behmard, Aida, Fayolle, Edith C., Graninger, Dawn M., Bergner, Jennifer B., Martín-Doménech, Rafael, Maksyutenko, Pavlo, Rajappan, Mahesh, Öberg, Karin I.
Small hydrocarbons are an important organic reservoir in protostellar and protoplanetary environments. Constraints on desorption temperatures and binding energies of such hydrocarbons are needed for accurate predictions of where these molecules exist
Externí odkaz:
http://arxiv.org/abs/1903.09720