Spitzer Space Telescope spectroscopy of ices toward low-mass embedded protostars

ACA Boogert*, KM Pontoppidan, F Lahuis, JK Jorgensen, JC Augereau, GA Blake, TY Brooke, CP Dullemond, NJ Evans, [No Value] Geers, MR Hogerheijde, J Kessler-Silacci, C Knez, P Morris, A Noriega-Crespo, FL Schoier, EF van Dishoeck, LE Allen, PM Harvey, DW KoernerLG Mundy, PC Myers, DL Padgett, AI Sargent, KR Stapelfeldt

*Corresponding author for this work

    Research output: Contribution to journalArticleAcademicpeer-review

    104 Citations (Scopus)


    Sensitive 5-38 mum Spitzer Space Telescope and ground-based 3-5 mum spectra of the embedded low-mass protostars B5 IRS1 and HH 46 IRS show deep ice absorption bands superposed on steeply rising mid-infrared continua. The ices likely originate in the circumstellar envelopes. The CO2 bending mode at 15 mum is a particularly powerful tracer of the ice composition and processing history. Toward these protostars, this band shows little evidence for thermal processing at temperatures above 50 K. Signatures of lower temperature processing are present in the CO and OCN- bands, however. The observed CO2 profile indicates an intimate mixture with H2O, but not necessarily with CH3OH, in contrast to some high-mass protostars. This is consistent with the low CH3OH abundance derived from the ground-based L-band spectra. The CO2: H2O column density ratios are high in both B5 IRS1 and HH 46 IRS (similar to35%). Clearly, the Spitzer spectra are essential for studying ice evolution in low-mass protostellar environments and for eventually determining the relation between interstellar and solar system ices.

    Original languageEnglish
    Pages (from-to)359-362
    Number of pages4
    JournalAstrophysical journal supplement series
    Issue number1
    Publication statusPublished - Sep-2004


    • astrochemistry
    • infrared : ISM
    • ISM : abundances
    • ISM : molecules
    • stars : formation
    • stars : individual (B5 IRS 1)
    • STARS
    • CO
    • CORES
    • DUST

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