2002ApJ...573L.123S


Query : 2002ApJ...573L.123S

2002ApJ...573L.123S - Astrophys. J., 573, L123-L127 (2002/July-2)

Proper motions in the knotty, bipolar jet in Henize 2-90.

SAHAI R., BRILLANT S., LIVIO M., GREBEL E.K., BRANDNER W., TINGAY S. and NYMAN L.-A.

Abstract (from CDS):

Using second-epoch Hubble Space Telescope imaging of the unusual, bipolar jet source He 2-90, we have discovered proper motions of 0".03 yr–1 in the jet knots. Combining the proper motion with the knots' radial velocity measured from ground-based long-slit data, we find that the jet speed is roughly 150-360 km.s–1, the source distance is 1-2.5 kpc, and the inclination (to the sky plane) of the jet axis is θ=10°-4°, although smaller values of θ and larger values of the jet speed and distance are not ruled out. A comparison of the [O III] and [N II] images shows the central obscuring disk structure directly. The disk, seen nearly edge-on, is embedded within a low-excitation circumstellar region extending from the equator up to a latitudinal angle of about ±62°, with the remaining latitudinal angular space being occupied by a biconical high-excitation region whose symmetry axis is aligned along the jet. The jet is at least 1400 yr old; the knots are being ejected at the rate of one pair roughly every 35-45 yr (independent of the tilt angle and distance to He 2-90), and accretion is still occurring since the youngest jet material is only ∼10 yr old. The jet can be plausibly driven by an accretion disk around a low-mass companion in an eccentric orbit with a period of ∼40 yr, with increased accretion during periastron passage producing the jet knots.

Abstract Copyright:

Journal keyword(s): Stars: Circumstellar Matter - ISM: Jets and Outflows - ISM: Planetary Nebulae: Individual: Alphanumeric: He 2-90 - Stars: AGB and Post-AGB - Stars: Mass Loss - Stars: Winds, Outflows

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 - 2024
#notes
1 WRAY 16-125 PN 13 09 36.2390615830 -61 19 35.976251345   14.508 13.517 13.568   B[e] 127 0

Query : 2002ApJ...573L.123S

Basic data :
WRAY 16-125 -- Planetary Nebula
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:
PN (1966PhDT,Hen,...), * (GSC2,LLNS,...), MIR (AKARI,MSX5C,...), AB? (1991A&AS), Em* ([W74]), G (ESO), NIR (2MASS), IR (IRAS)
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) :
13 09 36.2390615830 -61 19 35.976251345 (Optical) [ 0.2205 0.2823 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) :
13 06 26.9824247975 -61 03 37.257059140 [ 0.2205 0.2823 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) :
305.1099735452052 +01.4682398671881 [ 0.2205 0.2823 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 :
-6.297 -0.104 [0.277 0.348 90] 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:
B[e] D 2005A&A...441..289K
Syntax of angular size is : "maj-axis min-axis angle (wtype) quality bibcode"
  • maj-axis : major axis size (arc minutes)
  • min-axis : minor axis size (arc minutes)
  • angle : orientation angle (in degrees)
  • (wtype) : wavelength class for the origin of the angular size (Rad, mm, IR, Opt, UV, Xray, Gam)
  • quality : flag of quality of the angular size values ( A=best quality -> E=worst quality, {� } =unknown quality)
  • bibcode : bibcode of the angular size reference
Angular size (arcmin):
0.166666672 0.166666672 ~ (~) D 2010ApJ...714.1096S
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 (10) :
B 14.508 [0.02] E 2012yCat.1322....0Z
V 13.517 [0.01] E 2012yCat.1322....0Z
R 13.568 [0.07] E 2012yCat.1322....0Z
G 12.873022 [0.005479] C 2022yCat.1355....0G
J 10.870 [0.024] C 2003yCat.2246....0C
H 9.622 [0.024] C 2003yCat.2246....0C
K 7.930 [0.023] C 2003yCat.2246....0C
g 13.848 [0.01] E 2012yCat.1322....0Z
r 12.125 [0.01] E 2012yCat.1322....0Z
i 12.531 [0.01] E 2012yCat.1322....0Z
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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within arcsec The VizieR photometry tool allows for easy visualization of photometry points extracted around the Simbad position from photometry-enabled catalogues in VizieR.
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!).
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The link on the acronym of the identifiers give access to the information for this acronym in the dictionary of nomenclature.
Identifiers (19) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

ESO 132-1 LLNS 9924 PN Sa 2-90 WISE J130936.16-611935.7
AKARI-IRC-V1 J1309362-611935 2MASS J13093623-6119359 SCM 70 WRAY 16-125
GSC2 S212302116552 MSX5C G305.1103+01.4684 TIC 441479811 [W74] 43
Hen 2-90 PK 305+01 1 TYC 8990-3688-1 Gaia DR3 5863599857739835264
IRAS 13064-6103 PN G305.1+01.4 UCAC4 144-117912

References (127 between 1850 and 2024) (Total 127)
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 : 1    PM : 1   

   

Observing logs


herschel : 1    ISO : 3    IUE : 1   

   


External archives :

Data at NED - NASA/IPAC Extragalactic Database : WRAY 16-125

Link by name to the catalogue in VizieR :

AKARI-IRC-V1 J1309362-611935 IRAS 13064-6103 2MASS J13093623-6119359 MSX5C G305.1103+01.4684 PN G305.1+01.4
TYC 8990-3688-1 UCAC4 144-117912 WISE J130936.16-611935.7 Gaia DR3 5863599857739835264

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