2016ApJ...819...38C


Query : 2016ApJ...819...38C

2016ApJ...819...38C - Astrophys. J., 819, 38 (2016/March-1)

Chemical evolution of a CO ice induced by soft x-rays.

CIARAVELLA A., CHEN Y.-J., CECCHI-PESTELLINI C., JIMENEZ-ESCOBAR A., MUNOZ CARO G.M., CHUANG K.-J. and HUANG C.-H.

Abstract (from CDS):

We irradiated a pure carbon monoxide ice with soft X-rays of energies up to 1.2 keV. The experiments were performed using the spherical grating monochromator beamline at the National Synchrotron Radiation Research Center in Taiwan, exploiting both monochromatic (at 0.3 and 0.55 keV) and broader energy (0.25-1.2 keV) fluxes. The infrared spectra of the irradiated ices showed the formation of a number of products such as polycarbon mono- and dioxides CnOm, and chains containing up to 10 carbon atoms. While a gentle increase in the energy absorbed by the ice sample is reflected by an increase in the column densities of newly born species, such correlation breaks down at very high fluxes. In this regime the production yield falls down sharply by about a factor of 100. The refractory residue obtained in the broad energy irradiation is a ''compromise'' between those obtained with proton irradiation of C3O2 and CO ices in previous experiments. Finally, we discuss the possible implications for space chemistry

Abstract Copyright: ∼

Journal keyword(s): ISM: molecules - methods: laboratory: molecular - X-rays: ISM

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 V* DM Tau Or* 04 33 48.7336763736 +18 10 09.973460280 14.30 14.82 14.00     M2Ve 731 0

Query : 2016ApJ...819...38C

Basic data :
V* DM Tau -- Orion Variable
Other object types:
otypes_help
* (2019AJ,UCAC2,...), Y*O (2010ApJS), IR (IRAS,PSCz), TT* (1999AJ), Or* (2017ARep), Y*? (2018A&A), Em* (HBC), V* (V*), EmO (MHA), NIR (2MASS), MIR (WISE)
ICRS coord. (ep=J2000) :
04 33 48.7336763736 +18 10 09.973460280 (Optical) [ 0.0180 0.0096 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
04 30 54.6707882728 +18 03 56.915537593 [ 0.0180 0.0096 90 ]
Gal coord. (ep=J2000) :
179.2557188297592 -19.6110017435240 [ 0.0180 0.0096 90 ]
Proper motions mas/yr :
11.691 -18.292 [0.023 0.015 90] A 2020yCat.1350....0G
Radial velocity / Redshift / cz :
V(km/s) 18.3115 [0.0538] / z(spectroscopic) 0.000061 [0.000000] / cz 18.31 [0.05]
   (NIR) A 2022ApJS..259...35A
Parallaxes (mas):
6.9421 [0.0217] A 2020yCat.1350....0G
Spectral type:
M2Ve C 1977ApJ...214..747H
Fluxes (7) :
U 14.30 [~] C 2002yCat.2237....0D
B 14.82 [~] C 2002yCat.2237....0D
V 14.00 [~] C 2002yCat.2237....0D
G 13.095755 [0.004501] C 2020yCat.1350....0G
J 10.442 [0.022] C 2003yCat.2246....0C
H 9.757 [0.021] C 2003yCat.2246....0C
K 9.522 [0.020] C 2003yCat.2246....0C
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 3 : 2812 Display criteria :

Identifiers (19) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

UCAC2 38202732 HBC 62 PSCz P04309+1803 WISE J043348.73+181009.8
AP J04334871+1810099 IRAS 04309+1803 SV* SVS 1083 WISE J043348.73+181009.9
CSI+18-04309 2MASS J04334871+1810099 TIC 61259576 Gaia DR3 3314282402395528192
EPIC 247047380 MHA 257-6 UBV 4380 Gaia DR2 3314282402395528192
GCRV 55187 NSVS 9439120 V* DM Tau

References (731 between 1850 and 2026) (Total 731)
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 : 3    Distance : 2    Var : 4    Rot : 6    Fe/H : 5    Plx : 2    PM : 2    SpT : 2   

   

Observing logs
Herschel : 21    ISO : 1   

   


External archives :

Data at NED - NASA/IPAC Extragalactic Database : V* DM Tau

Link by name to the catalogue in VizieR :

UCAC2 38202732 AP J04334871+1810099 IRAS 04309+1803 2MASS J04334871+1810099 V* DM Tau
WISE J043348.73+181009.8 WISE J043348.73+181009.9 Gaia DR3 3314282402395528192 Gaia DR2 3314282402395528192

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