2015ApJ...801L..33H


Query : 2015ApJ...801L..33H

2015ApJ...801L..33H - Astrophys. J., 801, L33 (2015/March-2)

Why are dense planetary rings only found between 8 AU and 20 AU?

HEDMAN M.M.

Abstract (from CDS):

The recent discovery of dense rings around the Centaur Chariklo (and possibly Chiron) reveals that complete dense planetary rings are not only found around Saturn and Uranus, but also around small bodies orbiting in the vicinity of those giant planets. This report examines whether or not there could be a physical process that would make rings more likely to form or persist in this particular part of the outer solar system. Specifically, the ring material orbiting Saturn and Uranus appears to be much weaker than the material forming the innermost moons of Jupiter and Neptune. Also, the mean surface temperatures of Saturn's, Uranus's, and Chariklo's rings are all close to 70 K. Thus the restricted distribution of dense rings in our solar system may arise because icy materials are particularly weak around that temperature.

Abstract Copyright: ∼

Journal keyword(s): planet-disk interactions - planets and satellites: rings

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 ASAS J140748-3945.7 Y*O 14 07 47.9297625720 -39 45 42.767059968   13.56 12.31 11.91 10.92 K5IVe 84 0

Query : 2015ApJ...801L..33H

Basic data :
ASAS J140748-3945.7 -- Young Stellar Object
Other object types:
otypes_help
* (2016MNRAS,GSC,...), V* (ASAS,1SWASP,...), MIR (WISEA,WISE), Y*O (2012AJ), X (1RXS), NIR (2MASS)
ICRS coord. (ep=J2000) :
14 07 47.9297625720 -39 45 42.767059968 (Optical) [ 0.0115 0.0122 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
14 04 45.2788817938 -39 31 27.596168962 [ 0.0115 0.0122 90 ]
Gal coord. (ep=J2000) :
318.5315620098465 +20.7855341949544 [ 0.0115 0.0122 90 ]
Proper motions mas/yr :
-23.108 -21.048 [0.015 0.017 90] A 2020yCat.1350....0G
Radial velocity / Redshift / cz :
V(km/s) 5.904000 [0.151000] / z(spectroscopic) 0.000020 [0.000001] / cz 5.90 [0.15]
   (Opt) A 2021MNRAS.506..150B
Parallaxes (mas):
7.2351 [0.014] A 2020yCat.1350....0G
Spectral type:
K5IVe C 2012AJ....143...72M
Fluxes (11) :
B 13.56 [0.07] D 2012yCat.1322....0Z
V 12.31 [0.03] C 2012AJ....143...72M
R 11.91 [0.04] D 2012yCat.1322....0Z
G 11.927564 [0.003318] C 2020yCat.1350....0G
I 10.92 [0.03] C 2005yCat.2263....0D
J 9.997 [0.022] C 2003yCat.2246....0C
H 9.425 [0.023] C 2003yCat.2246....0C
K 9.257 [0.020] C 2003yCat.2246....0C
g 12.97 [0.03] D 2012yCat.1322....0Z
r 11.89 [0.05] D 2012yCat.1322....0Z
i 11.46 [0.03] D 2012yCat.1322....0Z
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 5
: 1
: 10017 Display criteria :

Identifiers (16) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

GSC 07807-00004 PPMX J140747.9-394542 UCAC2 14835467 WISEA J140747.90-394542.9
ASAS J140748-3945.7 1RXS J140746.9-394543 UCAC3 101-141675 WISE J140747.91-394542.9
GALAH 170218003701267 1SWASP J140747.93-394542.6 UCAC4 252-062736 Gaia DR3 6117085769513415168
2MASS J14074792-3945427 TIC 179367009 V* V1400 Cen Gaia DR2 6117085769513415168

References (84 between 1850 and 2026) (Total 84)
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 : 1    Fe/H : 3    Plx : 3    PM : 2    SpT : 1   

   


External archives :

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

Link by name to the catalogue in VizieR :

GSC 07807-00004 GALAH 170218003701267 2MASS J14074792-3945427 1RXS J140746.9-394543 UCAC2 14835467
UCAC3 101-141675 UCAC4 252-062736 V* V1400 Cen WISEA J140747.90-394542.9 WISE J140747.91-394542.9
Gaia DR3 6117085769513415168 Gaia DR2 6117085769513415168

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