2017MNRAS.465.2053V

Query : 2017MNRAS.465.2053V

2017MNRAS.465.2053V - Mon. Not. R. Astron. Soc., 465, 2053-2059 (2017/February-3)

Binary star influence on post-main-sequence multi-planet stability.

VERAS D., GEORGAKARAKOS N., DOBBS-DIXON I. and GANSICKE B.T.

Abstract (from CDS):

Nearly every star known to host planets will become a white dwarf, and nearly 100 planet-hosts are now known to be accompanied by binary stellar companions. Here, we determine how a binary companion triggers instability in otherwise unconditionally stable single-star two-planet systems during the giant branch and white dwarf phases of the planet host. We perform about 700 full-lifetime (14 Gyr) simulations with A0 and F0 primary stars and secondary K2 companions, and identify the critical binary distance within which instability is triggered at any point during stellar evolution. We estimate this distance to be about seven times the outer planet separation for circular binaries. Our results help characterize the fates of planetary systems, and in particular which ones might yield architectures which are conducive to generating observable metal pollution in white dwarf atmospheres.

Journal keyword(s): methods: numerical - celestial mechanics - minor planets, asteroids: general - planets and satellites: dynamical evolution and stability - white dwarfs - white dwarfs

Simbad objects: 1

Full paper

View the references in ADS

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	LBQS 1145+0145	WD*	11 48 33.6297189672	+01 28 59.420446860						DB	216	0

Query : 2017MNRAS.465.2053V

Basic data :

LBQS 1145+0145 -- White Dwarf

* (1992ApJS,EPIC,...), WD* (1992ApJS,WD), WD? (2018MNRAS), QSO (LBQS), EB* (2016AJ), Opt (SDSS)

11 48 33.6297189672 +01 28 59.420446860 (Optical) [ 0.0754 0.0600 90 ] A 2020yCat.1350....0G

11 45 59.9170490692 +01 45 40.291033773 [ 0.0754 0.0600 90 ]

269.8500485730851 +60.2522309712248 [ 0.0754 0.0600 90 ]

-43.664 -4.027 [0.105 0.075 90] A 2020yCat.1350....0G

6.8534 [0.0907] A 2020yCat.1350....0G

DB D 1992ApJS...78..409B

G 17.145735 [0.003365] C 2020yCat.1350....0G

u (AB) 16.832 [0.007] C 2008ApJS..175..297A

g (AB) 16.985 [0.004] C 2008ApJS..175..297A

r (AB) 17.288 [0.005] C 2008ApJS..175..297A

i (AB) 17.559 [0.007] C 2008ApJS..175..297A

z (AB) 17.822 [0.023] C 2008ApJS..175..297A

Overlay

points in this preview

2MASS DSS

All

(CDSPortal)

Send to

An access of full data is available using the icon Vizier near the identifier of the catalogue

`WD 1145+017`	`HE 1145+0145`	`SDSS J114833.62+012859.4`	`Gaia DR3 3796414192429498880`
`EPIC 201563164`	`LBQS 1145+0145`	`Gaia DR2 3796414192429498880`

References (216 between 1850 and 2026) (Total 216)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).

Follow new references on this object

Collections of Measurements

External archives :

Data at NED - NASA/IPAC Extragalactic Database : LBQS 1145+0145

Link by name to the catalogue in VizieR :

WD 1145+017 LBQS 1145+0145 SDSS J114833.62+012859.4 Gaia DR2 3796414192429498880 Gaia DR3 3796414192429498880

Search by coordinates in Vizier (radius: 5 arcsec)

Annotations :
Annotations allow a user to add a note or report an error concerning the astronomical object and its data. It requires registration to post a note. See description .
Please, have a look at Best practices. The list of all annotations to SIMBAD objects can be found here .

The annotation server is currently not available. Sorry for any inconvenience

To bookmark this query, right click on this link: simbad:objects in 2017MNRAS.465.2053V and select 'bookmark this link' or equivalent in the popup menu