CDS

2019A&A...629A.106A

C.D.S. - SIMBAD4 rel 1.7 - 2021.03.02CET12:09:46

2019A&A...629A.106A - Astronomy and Astrophysics, volume 629A, 106-106 (2019/9-1)

Photophoresis in the circumjovian disk and its impact on the orbital configuration of the Galilean satellites.

ARAKAWA S. and SHIBAIKE Y.

Abstract (from CDS):

Jupiter has four large regular satellites called the Galilean satellites: Io, Europa, Ganymede, and Callisto. The inner three of the Galilean satellites orbit in a 4:2:1 mean motion resonance; therefore their orbital configuration may originate from the stopping of the migration of Io near the bump in the surface density distribution and following resonant trapping of Europa and Ganymede. The formation mechanism of the bump near the orbit of the innermost satellite, Io, is not yet understood, however. Here, we show that photophoresis in the circumjovian disk could be the cause of the bump using analytic calculations of steady-state accretion disks. We propose that photophoresis in the circumjovian disk could stop the inward migration of dust particles near the orbit of Io. The resulting dust-depleted inner region would have a higher ionization fraction, and thus admit increased magnetorotational-instability-driven accretion stress in comparison to the outer region. The increase of the accretion stress at the photophoretic dust barrier would form a bump in the surface density distribution, halting the migration of Io.

Abstract Copyright: © ESO 2019

Journal keyword(s): accretion, accretion disks - planets and satellites: formation - planets and satellites: gaseous planets

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 - 2021 		#notes
1 V* HL Tau Or* 04 31 38.471952 +18 13 58.08504   15.89 14.49 14.39   K5 1240 0

    Equat.    Gal    SGal    Ecl

C.D.S. - SIMBAD4 rel 1.7 - 2021.03.02CET12:09:46

Available data : Basic data  •  Identifiers  •  Plot & images  •  Bibliography  •  Measurements  •  External archives  •  Notes  •  Annotations

Basic data :
V* HL Tau -- Variable Star of Orion Type
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: 		* (EPIC,GSC,...), X (XEST,2XMM,...), IR (2MASS,AKARI,...), ** (**,WDS), Y*O (2010ApJS,[GMM2009]), TT* (1999AJ), Or* (2012ApJ), V* (V*,AAVSO), smm (JCMTSE,JCMTSF), HH (HH), Em* (HBC), Rad (GBS)
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) : 		04 31 38.471952 +18 13 58.08504 (Optical) [ 27 103 90 ] B 2012yCat.1322....0Z
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) : 		04 28 44.439270 +18 07 36.08893 [ 27 103 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) : 		178.858958888 -19.972234828 [ 27 103 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 : 		4.2 -15.3 [3.2 6.9 90] C 2012yCat.1322....0Z
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: 		K5 D 2004ApJ...616..998W
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 (11) :
B 15.89 [0.11] D 2012yCat.1322....0Z
V 14.49 [0.06] D 2012yCat.1322....0Z
R 14.39 [0.18] E 2012yCat.1322....0Z
J 10.624 [0.042] C 2003yCat.2246....0C
H 9.171 [0.046] C 2003yCat.2246....0C
K 7.410 [0.017] C 2003yCat.2246....0C
u (AB) 16.887 [0.009] C 2009yCat.2294....0A
g 15.20 [0.06] D 2012yCat.1322....0Z
r 13.80 [0.07] D 2012yCat.1322....0Z
i 13.01 [0.08] D 2012yCat.1322....0Z
z (AB) 12.296 [0.002] C 2009yCat.2294....0A
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 4 : 2701 Display criteria :

The link on the acronym of the identifiers give access to the information for this acronym in the dictionary of nomenclature.
Identifiers (29) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

2MASS J04313843+1813576 HH 150 UCAC4 542-009387 [FGM2003] S19
** HER 10B JCMTSE J043138.3+181356 V* HL Tau [FK83] LDN 1551 11
AKARI-IRC-V1 J0431384+181357 JCMTSF J043138.3+181356 WDS J04317+1814B [GBA2007] 1319
EPIC 210690913 JP11 5275 WISE J043138.43+181357.5 [GMM2009] Tau L1551 2
GBS-VLA J043138.42+181357.3 SDSS J043138.46+181357.8 XEST 22-043 AAVSO 0425+18B
GSC 01269-01065 SSV LDN 1551 1 2XMM J043138.4+181357
Haro 6-14 TIC 353752575 [BFR2003] 35
HBC 49 UCAC2 38202581 [FGM2003] 29

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References (1240 between 1850 and 2021) (Total 1240)
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


MK : 2    V* : 1   

   

Observing logs


ISO : 8    herschel : 2    IUE : 4   

   

External archives :

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

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

Link by name to the catalogue in VizieR :

2MASS J04313843+1813576 AKARI-IRC-V1 J0431384+181357 GSC 01269-01065 SDSS J043138.46+181357.8 UCAC2 38202581
UCAC4 542-009387 V* HL Tau WDS J04317+1814B WISE J043138.43+181357.5

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2021.03.02-12:09:46

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