Spitzer space telescope spectroscopy of ices toward low-mass embedded protostars
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Spitzer space telescope spectroscopy of ices toward low-mass embedded protostars. / Boogert, A. C.Adwin; Pontoppidan, Klaus M.; Lahuis, Fred; Jørgensen, Jes K.; Augereau, Jean Charles; Blake, Geoffrey A.; Brooke, Timothy Y.; Brown, Joanna; Dullemond, C. P.; Evans, Neal J.; Geers, Vincent; Hogerheijde, Michiel R.; Kessler-Silacci, Jacqueline; Knez, Claudia; Morris, Pat; Noriega-Crespo, Alberto; Schöier, Fredrik L.; Van Dishoeck, Ewine F.; Allen, Lori E.; Harvey, Paul M.; Koerner, David W.; Mundy, Lee G.; Myers, Philip C.; Padgett, Deborah L.; Sargent, Anneila I.; Stapelfeldt, Karl R.
I: Astrophysical Journal, Supplement Series, Bind 154, Nr. 1, 01.09.2004, s. 359-362.Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › fagfællebedømt
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TY - JOUR
T1 - Spitzer space telescope spectroscopy of ices toward low-mass embedded protostars
AU - Boogert, A. C.Adwin
AU - Pontoppidan, Klaus M.
AU - Lahuis, Fred
AU - Jørgensen, Jes K.
AU - Augereau, Jean Charles
AU - Blake, Geoffrey A.
AU - Brooke, Timothy Y.
AU - Brown, Joanna
AU - Dullemond, C. P.
AU - Evans, Neal J.
AU - Geers, Vincent
AU - Hogerheijde, Michiel R.
AU - Kessler-Silacci, Jacqueline
AU - Knez, Claudia
AU - Morris, Pat
AU - Noriega-Crespo, Alberto
AU - Schöier, Fredrik L.
AU - Van Dishoeck, Ewine F.
AU - Allen, Lori E.
AU - Harvey, Paul M.
AU - Koerner, David W.
AU - Mundy, Lee G.
AU - Myers, Philip C.
AU - Padgett, Deborah L.
AU - Sargent, Anneila I.
AU - Stapelfeldt, Karl R.
PY - 2004/9/1
Y1 - 2004/9/1
N2 - Sensitive 5-38 μm Spitzer Space Telescope and ground-based 3-5 μm 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 μm 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 H 2O, 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 (∼35%). 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.
AB - Sensitive 5-38 μm Spitzer Space Telescope and ground-based 3-5 μm 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 μm 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 H 2O, 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 (∼35%). 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.
KW - Astrochemistry
KW - Infrared: ISM
KW - ISM: abundances
KW - ISM: molecules
KW - Stars: formation
KW - Stars: individual (B5 IRS 1)
UR - http://www.scopus.com/inward/record.url?scp=5644262716&partnerID=8YFLogxK
U2 - 10.1086/422556
DO - 10.1086/422556
M3 - Journal article
AN - SCOPUS:5644262716
VL - 154
SP - 359
EP - 362
JO - Astrophysical Journal
JF - Astrophysical Journal
SN - 0067-0049
IS - 1
ER -
ID: 234015961