CDS

2015A&A...577A..88R

Query : 2015A&A...577A..88R

2015A&A...577A..88R - Astronomy and Astrophysics, volume 577A, 88-88 (2015/5-1)

Stellar laboratories. V. The XeVI ultraviolet spectrum and the xenon abundance in the hot DO-type white dwarf RE 0503-289.

RAUCH T., HOYER D., QUINET P., GALLARDO M. and RAINERI M.

Abstract (from CDS):

For the spectral analysis of spectra of hot stars with a high resolution and high signal-to-noise ratio (S/N), advanced non-local thermodynamic equilibrium (NLTE) model atmospheres are mandatory. These are strongly dependent on the reliability of the atomic data that are used for their calculation. Reliable XeVI oscillator strengths are used to identify Xe lines in the ultraviolet spectrum of the DO-type white dwarf RE0503-289 and to determine its photospheric Xe abundance. We publish newly calculated oscillator strengths that are based on a recently measured XeVI laboratory line spectrum. These strengths were used to consider their radiative and collisional bound-bound transitions in detail in our NLTE stellar-atmosphere models to analyze XeVI lines exhibited in high-resolution and high S/N UV observations of RE0503-289 . We identify three hitherto unknown XeVI lines in the ultraviolet spectrum of RE0503-289 and confirm the previously measured photospheric Xe abundance of this white dwarf (log Xe=-4.2±0.6 by mass). Reliable measurements and calculations of atomic data are prerequisite for stellar-atmosphere modeling. Observed XeVI line profiles in the ultraviolet spectrum of the white dwarf RE0503-289 were well reproduced with the newly calculated XeVI oscillator strengths.

Abstract Copyright: ∼

Journal keyword(s): atomic data - line: identification - stars: abundances - stars: atmospheres - stars: individual: RE0503-289 - white dwarfs

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 - 2023 		#notes
1 MCT 0501-2858 WD* 05 03 55.5148810152 -28 54 34.631077500 12.29 13.55 13.58     DOZ 103 0

Query : 2015A&A...577A..88R

Basic data :
MCT 0501-2858 -- White Dwarf
Origin of the objects types :

(Ref) Object type as listed in the reference "Ref"
(acronym) Object type linked to the acronym according to the original reference
() Anterior to 2007, before we can link the objet type to a reference, or given by the CDS team in some particular cases

Other object types: 		UV (2EUVE,EUVE,...), WD* (1994MNRAS,WD), * (2013MNRAS,Gaia), X (RE,RX), WD? (2021MNRAS), PM* (2018yCat), V* (1SWASP), NIR (2MASS)
Syntax of coordinates is : "ra dec (wtype) [error ellipse] quality bibcode" :
  • ra dec : right ascension and declination (unit and frame defined according to your Output Options)
    Grey values are increasing the original precision due to the computation of frame transformations
  • (wtype) : wavelength class for the origin of the coordinates (Rad, mm, IR, Optical, UV, Xray, Gam)
  • [error ellipse] : measurement uncertainty, on (ra,dec) if the positional angle is 90 degrees, on (majaxis,minaxis) otherwise (in mas at defined epoch in the original catalogue),
    position angle (in degrees North celestial pole to East)
  • quality : flag of quality
    • E ≥ 10"
    • D : 1-10" (and some old data)
    • C : 0.1-1"
    • B : 0.01-0.1" + 2MASS, Tyc
    • A : VLBI, Hipparcos
  • bibcode : bibcode of the coordinates reference
ICRS coord. (ep=J2000) : 		05 03 55.5148810152 -28 54 34.631077500 (Optical) [ 0.0227 0.0273 90 ] A 2020yCat.1350....0G
Syntax of coordinates is : "ra dec (wtype) [error ellipse] quality bibcode" :
  • ra dec : right ascension and declination (unit and frame defined according to your Output Options)
    Grey values are increasing the original precision due to the computation of frame transformations
  • (wtype) : wavelength class for the origin of the coordinates (Rad, mm, IR, Optical, UV, Xray, Gam)
  • [error ellipse] : measurement uncertainty, on (ra,dec) if the positional angle is 90 degrees, on (majaxis,minaxis) otherwise (in mas at defined epoch in the original catalogue),
    position angle (in degrees North celestial pole to East)
  • quality : flag of quality
    • E ≥ 10"
    • D : 1-10" (and some old data)
    • C : 0.1-1"
    • B : 0.01-0.1" + 2MASS, Tyc
    • A : VLBI, Hipparcos
  • bibcode : bibcode of the coordinates reference
FK4 coord. (ep=B1950 eq=1950) : 		05 01 57.3008799459 -28 58 45.331916607 [ 0.0227 0.0273 90 ]
Syntax of coordinates is : "ra dec (wtype) [error ellipse] quality bibcode" :
  • ra dec : right ascension and declination (unit and frame defined according to your Output Options)
    Grey values are increasing the original precision due to the computation of frame transformations
  • (wtype) : wavelength class for the origin of the coordinates (Rad, mm, IR, Optical, UV, Xray, Gam)
  • [error ellipse] : measurement uncertainty, on (ra,dec) if the positional angle is 90 degrees, on (majaxis,minaxis) otherwise (in mas at defined epoch in the original catalogue),
    position angle (in degrees North celestial pole to East)
  • quality : flag of quality
    • E ≥ 10"
    • D : 1-10" (and some old data)
    • C : 0.1-1"
    • B : 0.01-0.1" + 2MASS, Tyc
    • A : VLBI, Hipparcos
  • bibcode : bibcode of the coordinates reference
Gal coord. (ep=J2000) : 		230.6717314020185 -34.9355298194296 [ 0.0227 0.0273 90 ]
Syntax of proper motions is : "pm-ra pm-dec [error ellipse] quality bibcode"
  • pm-ra : mu-ra*cos(dec) (expressed in the ICRS system in mas/yr)
  • pm-dec : mu-dec (expressed in the ICRS system in mas/yr)
  • [error ellipse] : error major axis and minor axis (in mas), orientation angle (in deg)
  • quality : flag of quality (A=best quality -> E=worst quality, {� } =unknown quality)
  • bibcode : bibcode of the proper motion reference
Proper motions mas/yr : 		76.715 72.251 [0.030 0.035 90] A 2020yCat.1350....0G
Syntax of parallax is : 'value quality [error] bibcode'
  • value : parallax value
  • quality : flag of quality (A=best quality -> E=worst quality, {� } =unknown quality)
  • [error] : mean error
  • bibcode : bibcode of the parallax reference
Parallaxes (mas): 		7.2332 [0.0325] A 2020yCat.1350....0G
Spectral type is made of 3 parts: %coding is composed of 4 parts :
  • the spectral type, which is made of a temperature class, eventually a luminosity class (roman number) and/or spectral peculiarities;
  • a quality letter: A=best quality→E=worst quality, {� } =unknown quality %
  • a quality letter: A=best quality -> E=worst quality, {� } =unknown quality
  • bibcode : bibcode of the spectral type reference
Spectral type: 		DOZ D 2021AJ....162..188B
Syntax of fluxes (or magnitudes) is : "filter-name (System) flux-value [error] quality MultVarFlags bibcode"
  • filter-name : U, B, V, R, I, G, J, H, K, u, g, r, i, z
  • (System) : may be AB (default is Vega)
  • flux-value : value of flux or magnitude
  • [error] : error value
  • quality : flag of quality of the flux value ( A=best quality -> E=worst quality, {� } =unknown quality)
  • MultVarFlags : Mult is zero or one char (J) for joined photometry ; Var can be zero or two chars (V[0-4])
  • bibcode : bibcode of the flux reference
Fluxes (7) :
U 12.29 [~] D 2013MNRAS.431..240O
B 13.55 [~] D 2013MNRAS.431..240O
V 13.58 [~] D 2011MNRAS.410..899F
G 13.824740 [0.002833] C 2020yCat.1350....0G
J 14.65 [0.03] C 2003yCat.2246....0C
H 14.77 [0.06] C 2003yCat.2246....0C
K 14.95 [0.14] D 2003yCat.2246....0C
SIMBAD within arcmin
', {sourceSize:12, color:'#30a090'})); aladin.on('objectClicked', function(object) { var objName=object.data.MAIN_ID; aladin.showPopup(object.ra,object.dec,'',''+ objName+''); });" title="Show Simbad objects"> Overlay Simbad points in this preview
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The search radius has to be specified by the user. It is currently limited to a maximum of 30 arcsec. It depends mostly on the precision or quality of the coordinates (SIMBAD and VizieR catalogs), the resolution of the images from which the sources were extracted, source extent, and source crowding.
Suggestions are: crowded field: 0.5 to 1.5 arcsec, 3 arcsec otherwise; uncertain coordinates (SIMBAD quality E or coordinates without reference): 5 to 30 arsec (risky!). sed-help-icon

The link on the acronym of the identifiers give access to the information for this acronym in the dictionary of nomenclature.
Identifiers (20) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

WD 0501-289 GALEX J050355.4-285432 RE J0503-28 1SWASP J050355.38-285436.0
EC 05019-2858 2MASS J05035551-2854345 RE J0503-285 TIC 13072717
2EUVE J0503-28.8 MCT 0501-2858 RE J0503-289 EQ 0501-289
EUVE J0503-28.8 2RE J050355-285456 RE J050353-285504 Gaia DR3 4876967941937370368
EUVE J0503-28.9 2RE J0503-285 RX J0503.9-2854 Gaia DR2 4876967941937370368

References (103 between 1850 and 2023) (Total 103)
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


distance : 2    Fe_H : 1    PLX : 2    PM : 2    MK : 3   

   

Observing logs


IUE : 11   

   

External archives :

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

Data at NED - NASA/IPAC Extragalactic Database : MCT 0501-2858

Link by name to the catalogue in VizieR :

WD 0501-289 EUVE J0503-28.8 EUVE J0503-28.9 GALEX J050355.4-285432 2MASS J05035551-2854345
2RE J050355-285456 2RE J0503-285 Gaia DR3 4876967941937370368 Gaia DR2 4876967941937370368

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2023.05.31-06:29:53

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