2017ApJ...843...25M

Query : 2017ApJ...843...25M

2017ApJ...843...25M - Astrophys. J., 843, 25-25 (2017/July-1)

Geodesic models of quasi-periodic-oscillations as probes of quadratic gravity.

MASELLI A., PANI P., COTESTA R., GUALTIERI L., FERRARI V. and STELLA L.

Abstract (from CDS):

Future very-large-area X-ray instruments (for which the effective area is larger than 3 m²) will be able to measure the frequencies of quasi-periodic oscillations (QPOs) observed in the X-ray flux from accreting compact objects with sub-percent precision. If correctly modeled, QPOs can provide a novel way to test the strong-field regime of gravity. By using the relativistic precession model and a modified version of the epicyclic resonance model, we develop a method to test general relativity against a generic class of theories with quadratic curvature corrections. With the instrumentation being studied for future missions such as eXTP, LOFT, or STROBE-X, a measurement of at least two QPO triplets from a stellar mass black hole can set stringent constraints on the coupling parameters of quadratic gravity.

Journal keyword(s): accretion, accretion disks - black hole physics - gravitation - X-rays: binaries - X-rays: binaries

Simbad objects: 1

Full paper

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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* V1033 Sco	HXB	16 54 00.1423963019	-39 50 44.761701340				16.14		F3-6IV	1980	0

Query : 2017ApJ...843...25M

Basic data :

V* V1033 Sco -- High Mass X-ray Binary

X (2008ApJ,PBC,...), * (UCAC4,ChOPS,...), LXB (2013ApJS), V* (V*,AAVSO), gam (GRO,INTREF), HXB (2012ApJ), No* (NOVA), NIR (2MASS)

16 54 00.1423963019 -39 50 44.761701340 (Optical) [ 0.0438 0.0276 90 ] A 2020yCat.1350....0G

16 50 33.1097810893 -39 45 52.417537282 [ 0.0438 0.0276 90 ]

344.9819404282615 +02.4559750537325 [ 0.0438 0.0276 90 ]

-4.329 -7.461 [0.062 0.047 90] A 2020yCat.1350....0G

0.2902 [0.0481] A 2020yCat.1350....0G

F3-6IV D 2008ApJ...685..463K

R 16.14 [0.01] C 2008ApJ...685..463K

G 16.226719 [0.005626] C 2022yCat.1355....0G

J 13.516 [0.029] C 2003yCat.2246....0C

H 12.997 [0.044] C 2003yCat.2246....0C

K 12.744 [0.034] C 2003yCat.2246....0C

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`UCAC4 251-103937`	`INTREF 727`	`SWIFT J1654.0-3950`	`AAVSO 1647-39`
`ChOPS J165400.14-395045.1`	`2MASS J16540014-3950447`	`TIC 339434742`	`Gaia DR3 5969790961312131456`
`GRO J1655-40`	`NOVA Sco 1994`	*`V V1033 Sco`**
`GRO J1655-44`	`PBC J1653.9-3950`	`2XMM J165400.1-395044`
`GRO J1655-41`	`SWIFT J1653.8-3952`	`[KRL2007b] 208`

References (1980 between 1850 and 2026) (Total 1980)
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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Archive data at HEASARC - High-Energy Astrophysics Science Archive Research Center

Data at NED - NASA/IPAC Extragalactic Database : V* V1033 Sco

Link by name to the catalogue in VizieR :

UCAC4 251-103937 2MASS J16540014-3950447 V* V1033 Sco Gaia DR3 5969790961312131456

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