2022MNRAS.517.1919R


Query : 2022MNRAS.517.1919R

2022MNRAS.517.1919R - Mon. Not. R. Astron. Soc., 517, 1919-1927 (2022/December-1)

Thermal desorption of H2O ice: from nanoscale films to the bulk.

ROSU-FINSEN A., CHIKANI B. and SALZMANN C.G.

Abstract (from CDS):

The desorption properties of H2O films are investigated across a wide range of film thicknesses from 53 nanometres (nm) to 101 micrometres (μm) using a quartz-crystal microbalance (QCM) and temperature-programmed desorption. Three desorption stages are observed belonging to amorphous solid water (ASW), stacking disordered ice I (ice Isd), and hexagonal ice I (ice Ih). The desorption of ASW is only detectable for the ≥10 μm films and is separated from the ice I desorption by 10-15 K with an associated desorption energy of ∼64 kJ mol–1. The desorption energy of the 53-nm film was found to be near 50 kJ mol–1 as also noted in the literature, but with increasing film thickness, the desorption energy of ice I rises, reaching a plateau around 65-70 kJ mol–1. The reason for the increased desorption energy is suggested to be due to molecules unable to desorb due to the thick covering layer of H2O and possibly re-adsorption events. Before complete desorption of ice I at around 220 K for the 101 μm film, a two-stage ice I desorption is observed with the QCM for the ≥10 μm films near 200 K. This event corresponds to the desorption of ice Isd as corroborated by X-ray diffraction patterns collected upon heating from 92 to 260 K at ambient pressure. Cubic ice is not observed as is commonly stated in the literature as resulting from the crystallization of ASW. Therefore, ice Isd is the correct terminology for the initial crystallization product of ASW.

Abstract Copyright: © The Author(s) 2022. Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): astrochemistry - ISM: molecules - methods: laboratory: molecular - methods: laboratory: solid state

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME LDN 1455 IRS 1 cor 03 27 39.08 +30 13 03.1           ~ 173 0

Query : 2022MNRAS.517.1919R

Basic data :
NAME LDN 1455 IRS 1 -- Dense Core
Other object types:
otypes_help
smm (JCMTLSG,JCMTSE,...), Y*O (2008ApJ,[EES2009],...), Y*? (2013ApJS,[HL2013],...), IR (IRAS,[BC86b],...), mm (2009ApJ,[EYG2006]), PoC ([KJD2006],[KJT2007]), cor (2008ApJ), X ([S2009]), MIR (SSTc2d)
ICRS coord. (ep=J2000) :
03 27 39.08 +30 13 03.1 (Infrared) [ 300 300 90 ] C 2009ApJS..181..321E
FK4 coord. (ep=B1950 eq=1950) :
03 24 34.98 +30 02 39.7 [ 300 300 90 ]
Gal coord. (ep=J2000) :
158.76708 -21.57564 [ 300 300 90 ]
VLSR :
4.926 4.526 5.326 [0.018] (mm) 2018ApJ...869...51I
Angular size (arcmin):
0.47 0.37 141 (smm) C 2019MNRAS.485.2895E
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 2
: 2
: 533 Display criteria :

Identifiers (25) :
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IRAS 03245+3002 SCOPE G158.77-21.58 [HFR2007] 35 [KJT2007] SMM 78
JCMTLSG J032739.2+301303 SSTc2d J032739.1+301303 [HL2013] 051.91284+30.21754 [KJT2007] SMM J032765+30130
JCMTSE J032739.2+301259 SSTc2d J032739.0+301303 [HRF2005] 35 [S2009] L1455 Object 11
JCMTSF J032739.2+301259 [BC86b] LDN 1455 IRS 1 [HSW2018] L1455-2 [TPB97] L 1455 FIR 4
NAME LDN 1455 IRS 1 [EDJ2009] 130 [JJK2007] 6
NAME RNO 15 FIR [EES2009] Per-emb 17 [KJD2006] SMM J032765+30130
NAME LDN 1455 FIR [EYG2006] Bolo 22 [KJT2007] 135

References (173 between 1850 and 2026) (Total 173)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Collections of Measurements Description of Measurements

Velocities : 2   

   

Observing logs
Herschel : 1    ISO : 3   

   


External archives :

Archive data at HEASARC - High-Energy Astrophysics Science Archive Research Center

Data at NED - NASA/IPAC Extragalactic Database : NAME LDN 1455 IRS 1

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IRAS 03245+3002

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