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20032024
most citedThe Spitzer ice legacy: Ice evolution from cores to protostars

570 citations · 4.6k across the 51 of their papers we have counts for

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9 papers · 1 filter

astro-ph2008★ 13 cited

Detection of CI in absorption towards PKS 1830-211 with the eSMA

Sandrine Bottinelli, A. Meredith Hughes, Ewine F. van Dishoeck +10

We report the first science observations and results obtained with the "extended" SMA (eSMA), which is composed of the SMA (Submillimeter Array), JCMT (James Clerk Maxwell Telescop…

astro-ph2008★ 5 cited

The eSMA: description and first results

Sandrine Bottinelli, Ken H. Young, Richard Chamberlin +15

The eSMA ("extended SMA") combines the SMA, JCMT and CSO into a single facility, providing enhanced sensitivity and spatial resolution owing to the increased collecting area at the…

astro-ph2008★ 194 cited

The c2d Spitzer spectroscopy survey of ices around low-mass young stellar objects, III: CH4

Karin I. Oberg, A. C. Adwin Boogert, Klaus M. Pontoppidan +4

CH4 is proposed to be the starting point of a rich organic chemistry. Solid CH4 abundances have previously been determined mostly toward high mass star forming regions. Spitzer/IRS…

astro-ph2008★ 384 cited

The c2d Spitzer Spectroscopic Survey of Ices Around Low-Mass Young Stellar Objects: I. H2O and the 5-8 um Bands

A. Boogert, K. Pontoppidan, C. Knez +23

With the goal to study the physical and chemical evolution of ices in solar-mass systems, a spectral survey is conducted of a sample of 41 low luminosity YSOs using 3-38 um Spitzer…

astro-ph2006★ 189 cited

Hot corinos in NGC1333-IRAS4B and IRAS2A

Sandrine Bottinelli, Cecilia Ceccarelli, Jonathan P. Williams +1

(Abridged) We aim to enlarge the number of known hot corinos and carry out a first comparative study with hot cores. The ultimate goal is to understand whether complex organic mole…

astro-ph2004★ 203 cited

Near-arcsecond resolution observations of the hot corino of the solar type protostar IRAS 16293-2422

Sandrine Bottinelli, Cecilia Ceccarelli, Roberto Neri +6

Complex organic molecules have previously been discovered in solar type protostars, raising the questions of where and how they form in the envelope. Possible formation mechanisms…