Experimental study of gas phase titanium and aluminum oxide clusters

被引:55
作者
Demyk, K
van Heijnsbergen, D
von Helden, G
Meijer, G
机构
[1] EURATOM, FOM, Inst Plasmaphys Rijnhuizen, NL-3439 MN Nieuwegein, Netherlands
[2] Univ Nijmegen, Dept Mol & Laser Phys, NL-6525 ED Nijmegen, Netherlands
[3] Max Planck Gesell, Fritz Haber Inst, D-14195 Berlin, Germany
关键词
methods : laboratory; ISM; dust; extinction;
D O I
10.1051/0004-6361:20034117
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present an experimental study of the vibrational properties of gas phase titanium oxide and aluminum oxide clusters. The titanium and aluminum oxide clusters have a stoichiometry of (Ti2O3)(x)-(TiO2)(y) (with (x, y) from (2, 4) to (11, 29)) and AlO-(Al2O3)(n) (5 less than or equal to n less than or equal to 70). The vibrational properties of the clusters are obtained using infrared resonance enhanced multi-photon ionization (IR-REMPI) spectroscopy. Titanium oxide clusters have a strong vibrational band at similar to13.5 mum, suggesting that their structure is close to the rutile bulk phase of TiO2. Aluminum oxide clusters seem to have a structure comparable to the bulk gamma-Al2O3; their IR-REMPI spectra exhibit a vibrational band at similar to11 mum and another band at similar to15 mum which appears in the spectra of clusters containing more than 7-8 Al atoms and becomes more intense as the cluster size increases. As hot neutral clusters are observed to evaporate more easily electrons than neutral fragments, one can conclude that they are very stable and thus very good nucleation seeds for dust growth.
引用
收藏
页码:547 / 552
页数:6
相关论文
共 33 条
[1]  
Bohren C., 1983, ABSORPTION SCATTERIN
[2]  
DESERT FX, 1990, ASTRON ASTROPHYS, V237, P215
[3]   The 3.3 micron and extended red emissions in interstellar clouds: Further evidence for carbon nanoparticles [J].
Duley, WW .
ASTROPHYSICAL JOURNAL, 2001, 553 (02) :575-580
[4]   Mineral formation in stellar winds - III. Dust formation in S stars [J].
Ferrarotti, AS ;
Gail, HP .
ASTRONOMY & ASTROPHYSICS, 2002, 382 (01) :256-281
[5]   Phonons of clean and metal-modified oxide films:: an infrared and HREELS study [J].
Frank, M ;
Wolter, K ;
Magg, N ;
Heemeier, M ;
Kühnemuth, R ;
Bäumer, M ;
Freund, HJ .
SURFACE SCIENCE, 2001, 492 (03) :270-284
[6]   Inorganic dust formation in astrophysical environments [J].
Gail, HP ;
Sedlmayr, E .
FARADAY DISCUSSIONS, 1998, 109 :303-319
[7]  
GAIL HP, 1999, ASTRON ASTROPHYS, V347, P549
[8]  
Gervais F., 1991, HDB OPTICAL CONSTANT, VII, P761
[9]   Theoretical structure determination of γ-Al2O3 -: art. no. 012101 [J].
Gutiérrez, G ;
Taga, A ;
Johansson, B .
PHYSICAL REVIEW B, 2002, 65 (01) :1-4
[10]  
Hill HGM, 1998, ASTRON ASTROPHYS, V336, pL41