2018MNRAS.480.1898C


Query : 2018MNRAS.480.1898C

2018MNRAS.480.1898C - Mon. Not. R. Astron. Soc., 480, 1898-1911 (2018/October-3)

Accretion in common envelope evolution.

CHAMANDY L., FRANK A., BLACKMAN E.G., CARROLL-NELLENBACK J., LIU B., TU Y., NORDHAUS J., CHEN Z. and PENG B.

Abstract (from CDS):

Common envelope evolution (CEE) is presently a poorly understood, yet critical, process in binary stellar evolution. Characterizing the full 3D dynamics of CEE is difficult in part because simulating CEE is so computationally demanding. Numerical studies have yet to conclusively determine how the envelope ejects and a tight binary results, if only the binary potential energy is used to propel the envelope. Additional power sources might be necessary and accretion onto the inspiraling companion is one such source. Accretion is likely common in post-asymptotic giant branch binary interactions but how it operates and how its consequences depend on binary separation remain open questions. Here we use high-resolution global 3D hydrodynamic simulations of CEE with the adaptive mesh refinement code ASTROBEAR, to bracket the range of CEE companion accretion rates by comparing runs that remove mass and pressure via a subgrid accretion model with those that do not. The results show that if a pressure release valve is available, super-Eddington accretion may be common. Jets are a plausible release valve in these environments, and they could also help unbind and shape the envelopes.

Abstract Copyright: © 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): accretion, accretion discs - hydrodynamics - methods: numerical - binaries: close - stars: kinematics and dynamics

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 IRAS 19417+1701 RS* 19 43 59.5114618200 +17 09 00.963778248   11.2   10.6   ~ 71 0

Query : 2018MNRAS.480.1898C

Basic data :
IRAS 19417+1701 -- RS CVn Variable
Other object types:
otypes_help
PN (2011MNRAS,PN), MIR (AKARI,WISEA,...), * (USNO,Gaia), RS* (2020ApJS), ** (2011MNRAS), ISM (IPHASX), IR (IRAS)
ICRS coord. (ep=J2000) :
19 43 59.5114618200 +17 09 00.963778248 (Optical) [ 0.0649 0.0762 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
19 41 44.2421875415 +17 01 46.283523315 [ 0.0649 0.0762 90 ]
Gal coord. (ep=J2000) :
054.1614492103726 -03.3734577770215 [ 0.0649 0.0762 90 ]
Proper motions mas/yr :
-1.321 -3.942 [0.089 0.109 90] A 2020yCat.1350....0G
Parallaxes (mas):
0.1714 [0.0984] A 2020yCat.1350....0G
Angular size (arcmin):
0.35 0.35 90 (Opt) D 2014MNRAS.443.3388S
Fluxes (4) :
B 11.2 [~] E 2003AJ....125..984M
R 10.6 [~] E 2003AJ....125..984M
G 17.694447 [0.026675] C 2020yCat.1350....0G
g 17.789 [~] D 2020ApJS..249...18C
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Identifiers (13) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

AKARI-FIS-V1 J1943591+170903 NAME Necklace WISEA J194359.51+170900.9 Gaia DR3 1820974088126464384
IPHASX J194359.5+170901 NAME Necklace Nebula WISE J194359.51+170901.1
IPHASX J194359.5-170901 PN G054.2-03.4 ZTF J194359.50+170901.0
IRAS 19417+1701 USNO-B1.0 1071-00528101 Gaia DR2 1820974088126464384

References (71 between 1850 and 2026) (Total 71)
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

Var : 2    Plx : 2    PM : 2   

   


External archives :

Data at NED - NASA/IPAC Extragalactic Database : IRAS 19417+1701

Link by name to the catalogue in VizieR :

AKARI-FIS-V1 J1943591+170903 IRAS 19417+1701 PN G054.2-03.4 USNO-B1.0 1071-00528101 WISEA J194359.51+170900.9
WISE J194359.51+170901.1 Gaia DR2 1820974088126464384 Gaia DR3 1820974088126464384

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