On the origin of infrared bands attributed to tryptophan in Spitzer observations of IC 348

Détail du document

Identifiant

oai:arXiv.org:2405.16773

Sujet

Astrophysics - Astrophysics of Gal... Astrophysics - Solar and Stellar A...

Auteur

Dhariwal, Aditya Speak, Thomas H. Zeng, Linshan Rashidi, Amirhossein Moore, Brendan Berné, Olivier Remijan, Anthony J. Schroetter, Ilane McGuire, Brett A. Rivilla, Víctor M. Belloche, Arnaud Jørgensen, Jes K. Djuricanin, Pavle Momose, Takamasa Cooke, Ilsa R.

Catégorie

sciences : astrophysique

Année

2024

Date de référencement

29/05/2024

Mots clés

infrared spectra astrophysics data tryptophan

Métrique

Résumé

Infrared emission features toward interstellar gas of the IC 348 star cluster in Perseus have been recently proposed to originate from the amino acid tryptophan.

The assignment was based on laboratory infrared spectra of tryptophan pressed into pellets, a method which is known to cause large frequency shifts compared to the gas phase.

We assess the validity of the assignment based on the original Spitzer data as well as new data from JWST.

In addition, we report new spectra of tryptophan condensed in para-hydrogen matrices to compare with the observed spectra.

The JWST MIRI data do not show evidence for tryptophan, despite deeper integration toward IC 348.

In addition, we show that several of the lines attributed to tryptophan are likely due to instrumental artifacts.

This, combined with the new laboratory data, allows us to conclude that there is no compelling evidence for the tryptophan assignment.

Dhariwal, Aditya,Speak, Thomas H.,Zeng, Linshan,Rashidi, Amirhossein,Moore, Brendan,Berné, Olivier,Remijan, Anthony J.,Schroetter, Ilane,McGuire, Brett A.,Rivilla, Víctor M.,Belloche, Arnaud,Jørgensen, Jes K.,Djuricanin, Pavle,Momose, Takamasa,Cooke, Ilsa R., 2024, On the origin of infrared bands attributed to tryptophan in Spitzer observations of IC 348

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