Universität zu Köln

Nazari, P., Meijerhof, J. D., van Gelder, M. L., Ahmadi, A., van Dishoeck, E. F., Tabone, B., Langeroodi, D., Ligterink, N. F. W., Jaspers, J., Beltran, M. T., Fuller, G. A., Sanchez-Monge, A. and Schilke, P. (2022). N-bearing complex organics toward high-mass protostars Constant ratios pointing to formation in similar pre-stellar conditions across a large mass range. Astron. Astrophys., 668. LES ULIS CEDEX A: EDP SCIENCES S A. ISSN 1432-0746

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Abstract

Context. Complex organic species are known to be abundant toward low- and high-mass protostars. No statistical study of these species toward a large sample of high-mass protostars with the Atacama Large Millimeter/submillimeter Array (ALMA) has been carried out so far. Aims. We aim to study six N-bearing species: methyl cyanide (CH3CN), isocyanic acid (HNCO), formamide (NH2CHO), ethyl cyanide (C2H5CN), vinyl cyanide (C2H3CN) and methylamine (CH3NH2) in a large sample of line-rich high-mass protostars. Methods. From the ALMA Evolutionary study of High Mass Protocluster Formation in the Galaxy survey, 37 of the most line-rich hot molecular cores with similar to 1 angular resolution are selected. Next, we fit their spectra and find column densities and excitation temperatures of the N-bearing species mentioned above, in addition to methanol (CH3OH) to be used as a reference species. Finally, we compare our column densities with those in other low- and high-mass protostars.Results. CH3OH, CH3CN and HNCO are detected in all sources in our sample, whereas C2H3CN and CH3NH2 are (tentatively) detected in similar to 78 and similar to 32% of the sources. We find three groups of species when comparing their excitation temperatures: hot (NH2CHO; T-ex greater than or similar to 250 K), warm (C2H3CN, (HNCO)-C-13 and (CH3CN)-C-13; 100 K less than or similar to T-ex less than or similar to 250 K) and cold species (CH3OH and CH3NH2; T-ex less than or similar to 100 K). This temperature segregation reflects the trend seen in the sublimation temperature of these molecules and validates the idea that complex organic emission shows an onion-like structure around protostars. Moreover, the molecules studied here show constant column density ratios across low- and high-mass protostars with scatter less than a factor similar to 3 around the mean. Conclusions. The constant column density ratios point to a common formation environment of complex organics or their precursors, most likely in the pre-stellar ices. The scatter around the mean of the ratios, although small, varies depending on the species considered. This spread can either have a physical origin (source structure, line or dust optical depth) or a chemical one. Formamide is most prone to the physical effects as it is tracing the closest regions to the protostars, whereas such effects are small for other species. Assuming that all molecules form in the pre-stellar ices, the scatter variations could be explained by differences in lifetimes or physical conditions of the pre-stellar clouds. If the pre-stellar lifetimes are the main factor, they should be similar for low- and high-mass protostars (within factors similar to 2-3).

Item Type:	Journal Article
Creators:	Creators Email ORCID ORCID Put Code Nazari, P. UNSPECIFIED UNSPECIFIED UNSPECIFIED Meijerhof, J. D. UNSPECIFIED UNSPECIFIED UNSPECIFIED van Gelder, M. L. UNSPECIFIED UNSPECIFIED UNSPECIFIED Ahmadi, A. UNSPECIFIED UNSPECIFIED UNSPECIFIED van Dishoeck, E. F. UNSPECIFIED UNSPECIFIED UNSPECIFIED Tabone, B. UNSPECIFIED UNSPECIFIED UNSPECIFIED Langeroodi, D. UNSPECIFIED UNSPECIFIED UNSPECIFIED Ligterink, N. F. W. UNSPECIFIED UNSPECIFIED UNSPECIFIED Jaspers, J. UNSPECIFIED UNSPECIFIED UNSPECIFIED Beltran, M. T. UNSPECIFIED UNSPECIFIED UNSPECIFIED Fuller, G. A. UNSPECIFIED UNSPECIFIED UNSPECIFIED Sanchez-Monge, A. UNSPECIFIED UNSPECIFIED UNSPECIFIED Schilke, P. UNSPECIFIED UNSPECIFIED UNSPECIFIED
URN:	urn:nbn:de:hbz:38-692325
DOI:	10.1051/0004-6361/202243788
Journal or Publication Title:	Astron. Astrophys.
Volume:	668
Date:	2022
Publisher:	EDP SCIENCES S A
Place of Publication:	LES ULIS CEDEX A
ISSN:	1432-0746
Language:	English
Faculty:	Unspecified
Divisions:	Unspecified
Subjects:	no entry
Uncontrolled Keywords:	Keywords Language SUBMILLIMETER-WAVE SPECTRUM; CENTRIFUGAL-DISTORTION CONSTANTS; EXPLORING MOLECULAR COMPLEXITY; GROUND-STATE CONSTANTS; GAS-PHASE FORMATION; MSX SOURCE SURVEY; ROTATIONAL SPECTRUM; MICROWAVE-SPECTRUM; LINE SURVEY; INTERSTELLAR ICE Multiple languages Astronomy & Astrophysics Multiple languages
URI:	http://kups.ub.uni-koeln.de/id/eprint/69232