Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005a%26a...444l..57d&link_type=abstract
Astronomy and Astrophysics, Volume 444, Issue 3, December IV 2005, pp.L57-L60
Astronomy and Astrophysics
Astrophysics
7
Astrochemistry, Line: Identification, Ism: Dust, Extinction, Ism: Molecules, Ism: Lines And Bands, Ism: Individual: L723
Scientific paper
The L723 low mass class 0 protostellar object has been observed with the IRS low resolution spectrometer onboard Spitzer Space Telescope. A huge CO2 ice column density of 6.3 ± 1 × 1018 cm-2 is detected toward this extremely red object. We constructed the spectral energy distribution (SED) of L723 by combining the Spitzer spectral data with Infrared Space Observatory (ISO) camera extracted fluxes, IRAS points, ISO long wavelength spectrometer (LWS) observations and millimeter ground based observations. A self consistent 1D model was developed to fit the SED. We show that, besides the high CO2 column density, the abundance ratio of CO2 ice to silicates grain cores is similar to other lines-of-sight.
Dartois Emmanuel
Muñoz Caro Guillermo Manuel
Pontoppidan Klaus
Thi Wing-Fai
No associations
LandOfFree
Spitzer's large CO2 ice detection toward the L723 class 0 object does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Spitzer's large CO2 ice detection toward the L723 class 0 object, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spitzer's large CO2 ice detection toward the L723 class 0 object will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1276463