2000A&A...364..282F


Query : 2000A&A...364..282F

2000A&A...364..282F - Astronomy and Astrophysics, volume 364282-292 (2000/12-1)

Steps toward interstellar silicate mineralogy. V. Thermal Evolution of Amorphous Magnesium Silicates and Silica.

FABIAN D., JAEGER C., HENNING T., DORSCHNER J. and MUTSCHKE H.

Abstract (from CDS):

The thermally induced amorphous-to-crystalline transition has been studied for bulk sheets and micrometre-sized particles of magnesium silicate glass (MgSiO3), nanometre-sized amorphous magnesium silicate (MgSiO3 and Mg2SiO4 smokes) and amorphous silica particles (SiO2). Silicate glass was produced by the shock-quenching of melts. Samples of nanometre-sized smoke particles have been obtained by the laser ablation technique. Both the MgSiO3 and the Mg2SiO4 smokes have been found to consist of two particle species; particles of smaller size ranging in diametre from 10nm to about 100nm and bigger size ranging from a few 100nm to almost 3 micrometres in diametre. Nanometre-sized particles have been shown to be depleted in magnesium whereas the micrometre-sized particles were found to be enriched in Mg. Generally, the particles are composed of nonstoichiometric magnesium silicates with compositions varying even inside of the particles. Frequently, the particles contained internal voids that are assumed to have been formed by thermal shrinkage or outgassing of the particles' interior during cooling. Annealing at 1000K transformed the magnesium silicate smokes into crystalline forsterite (c-Mg2SiO4), tridymite (a crystalline modification of SiO2) and amorphous silica (a-SiO2) according to the initial Mg/Si-ratio of the smoke. Crystallization took place within a few hours for the Mg2SiO4 smoke and within one day for the MgSiO3 smoke. The MgSiO3 glass evolved more slowly because crystallization started at the sample surface. It has been annealed at temperatures ranging from 1000 to 1165K. In contrast to the smoke samples, MgSiO3 glass crystallized as orthoenstatite (MgSiO3). Only after 50 hours of annealing at 1000K, weak indications of forsterite and tridymite formation have been found in the X-ray diffraction spectra. At a temperature of 1000K, amorphous silica nanoparticles showed distinctly lower rates of thermal evolution compared with the magnesium silicates. At 1220K, the timescale of crystallization of a-SiO2 into cristobalite and tridymite amounts to 4.5 h. From the experiments, crystallization parameters have been obtained: activation energy and velocity of crystal growth. The spectra shown in this study will be made publically available in the electronic database (http://www.astro.uni-jena.de).

Abstract Copyright: ∼

Journal keyword(s): stars: circumstellar matter - stars: formation - stars: AGB and post-AGB - solar system: formation - methods: laboratory

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 HD 142527 Ae* 15 56 41.8882637904 -42 19 23.248281828   9.04 8.34     F6III 741 1

Query : 2000A&A...364..282F

Basic data :
HD 142527 -- Herbig Ae/Be Star
Other object types:
otypes_help
* (2022ApJS,HD,...), MIR (AKARI,WISEA,...), ** (**,WDS), Ae* (2014MNRAS), Or* (2023A&A), Y*O (2016A&A), Y*? (2020AJ), Em* (Hen), NIR (2MASS), IR (IRAS)
ICRS coord. (ep=J2000) :
15 56 41.8882637904 -42 19 23.248281828 (Optical) [ 0.0222 0.0160 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
15 53 16.2710486016 -42 10 41.791426678 [ 0.0222 0.0160 90 ]
Gal coord. (ep=J2000) :
335.6548694314286 +08.4804092143173 [ 0.0222 0.0160 90 ]
Proper motions mas/yr :
-10.924 -26.149 [0.028 0.022 90] A 2020yCat.1350....0G
Radial velocity / Redshift / cz :
V(km/s) -0.23 [1.18] / z(spectroscopic) -0.000001 [0.000004] / cz -0.23 [1.18]
   (Opt) B 2018yCat.1345....0G
Parallaxes (mas):
6.2791 [0.0284] A 2020yCat.1350....0G
Spectral type:
F6III C 1978MSS...C02....0H
Angular size (arcmin):
0.0017 0.0 133 (Opt) C 2014ApJ...781L..30C
Fluxes (6) :
B 9.04 [0.02] D 2000A&A...355L..27H
V 8.34 [0.01] D 2000A&A...355L..27H
G 8.114528 [0.002841] C 2020yCat.1350....0G
J 6.503 [0.029] C 2003yCat.2246....0C
H 5.715 [0.031] C 2003yCat.2246....0C
K 4.980 [0.020] C 2003yCat.2246....0C
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 3
: 1
: 322 Display criteria :

Identifiers (24) :
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HD 142527 CPD-41 7393 IRAS 15532-4210 uvby98 100142527
** BIL 5 GEN# +1.00142527 2MASS J15564188-4219232 WDS J15567-4219AB
AKARI-IRC-V1 J1556418-421921 GSC 07846-00688 PPM 321217 WISEA J155641.87-421923.4
AKARI-FIS-V1 J1556415-421932 Hen 3-1119 SAO 226389 WISE J155641.87-421923.7
CD-41 10447 HIC 78092 TIC 255191560 Gaia DR3 5994826707951507200
CPC 0 14212 HIP 78092 TYC 7846-688-1 Gaia DR2 5994826707951507200

References (741 between 1850 and 2026) (Total 741)
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 : 4    Distance : 3    Rot : 2    Fe/H : 3    Plx : 4    PM : 5    SpT : 3   

   

Observing logs
Herschel : 9    ISO : 3   

   


External archives :

Data at NED - NASA/IPAC Extragalactic Database : HD 142527

Link by name to the catalogue in VizieR :

HD 142527 AKARI-IRC-V1 J1556418-421921 AKARI-FIS-V1 J1556415-421932 CD-41 10447 CPD-41 7393
GSC 07846-00688 HIC 78092 HIP 78092 IRAS 15532-4210 2MASS J15564188-4219232
PPM 321217 SAO 226389 TYC 7846-688-1 uvby98 100142527 WDS J15567-4219AB
WISEA J155641.87-421923.4 WISE J155641.87-421923.7 Gaia DR3 5994826707951507200 Gaia DR2 5994826707951507200

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