2019ApJS..240...36H

Query : 2019ApJS..240...36H

2019ApJS..240...36H - Astrophys. J., Suppl. Ser., 240, 36-36 (2019/February-0)

Bolometric treatment of irradiation effects: general discussion and application to binary stars.

HORVAT M., CONROY K.E., JONES D. and PRSA A.

Abstract (from CDS):

A general framework for dealing with irradiation effects in the bolometric sense-specifically, reflection with heat absorption and the consequent redistribution of the absorbed heat-for systems of astrophysical bodies where the boundaries are used as support for the description of the processes, is presented. Discussed are its mathematical and physical properties, as well as its implementation approximations, with a focus on three plausible redistribution processes (uniform, latitudinal, and local redistribution). These are tested by extending PHOEBE 2.1 (http://phoebe-project.org/), the open-source package for modeling eclipsing binaries, and applied to a toy model of the known two-body eclipsing systems.

Journal keyword(s): binaries: eclipsing - methods: analytical - methods: numerical - stars: fundamental parameters - techniques: photometric

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	V* NN Ser	RS*	15 52 56.1203524080	+12 54 44.429312196			16.51			DAO1+M4	287	0

Query : 2019ApJS..240...36H

Basic data :

V* NN Ser -- RS CVn Variable

WD? (2019MNRAS), V* (2018AJ,V*), * ([HH95],Gaia), MIR (WISEA,WISE), CV* (2017ARep), WD* (WD), RS* (2020ApJS), EB* (2014ApJS), UV (PG), NIR (2MASS), Opt (ATO)

15 52 56.1203524080 +12 54 44.429312196 (Optical) [ 0.0497 0.0557 90 ] A 2020yCat.1350....0G

15 50 35.5074124438 +13 03 39.305144353 [ 0.0497 0.0557 90 ]

023.6529230497113 +45.3388622667198 [ 0.0497 0.0557 90 ]

-30.170 -59.084 [0.055 0.057 90] A 2020yCat.1350....0G

1.9438 [0.0662] A 2020yCat.1350....0G

DAO1+M4 C 2010MNRAS.402.2591P

V 16.51 [~] V3 D 2014ApJS..213....9D

G 16.531082 [0.014687] C 2020yCat.1350....0G

J 16.907 [0.163] D 2003yCat.2246....0C

H 16.254 [0.204] D 2003yCat.2246....0C

K 16.168 [0.286] D 2003yCat.2246....0C

g 16.429 [~] D 2020ApJS..249...18C

r 16.749 [~] D 2020ApJS..249...18C

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`2MASS J15525613+1254446`	`PTF1 J155256.11+125443.9`	`WISEA J155256.11+125443.6`	`Gaia DR3 1191504471436192512`
`ATO J238.2337+12.9121`	`TIC 172608008`	`WISE J155256.12+125443.4`	`Gaia DR2 1191504471436192512`
`CRTS J155256.0+125444`	*`V NN Ser`**	`ZTF J155256.08+125443.4`
`PG 1550+131`	`WD 1550+130`	`[HH95] NN Ser-9`

References (287 between 1850 and 2026) (Total 287)
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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`2MASS J15525613+1254446`	`PG 1550+131`	*`V NN Ser`**	`WD 1550+130`	`WISEA J155256.11+125443.6`
`WISE J155256.12+125443.4`	`Gaia DR3 1191504471436192512`	`Gaia DR2 1191504471436192512`

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