2005A&A...429L..33N


C.D.S. - SIMBAD4 rel 1.7 - 2021.03.01CET09:25:52

2005A&A...429L..33N - Astronomy and Astrophysics, volume 429, L33-36 (2005/1-2)

Using close stars as probes of hot accretion flow in Sgr A*.

NAYAKSHIN S.

Abstract (from CDS):

The extremely hot and tenuous accretion flow in the immediate vicinity of Sgr A* is believed to be invisible (too dim) in the X-ray band, except for short X-ray flares. Here we point out that during pericenter passages, close brightest stars irradiate the inner region of the accretion flow, providing a plenty of optical/UV photons. These seed photons are Compton up-scattered by the hot electrons of the accretion flow to higher frequencies, some into the X-ray band, potentially making the innermost accretion flow much brighter in X-rays than usual. We propose to use coordinated near infra-red and X-ray observations of close star passages to put constraints onto Sgr A* accretion theories. The absence of a noticeable change in the steady emission of Sgr A* as observed by Chandra in the year 2002, when the star named S2 passed through a pericenter of its orbit, already rules out the hotter of the ``standard'' Advection-Dominated Accretion Flows. The less dense accretion flows, in particular the model of Yuan et al. (2003ApJ...598..301Y), passes the test and is constrained to accretion rates no larger than ∼few x10–7M/year.

Abstract Copyright:

Journal keyword(s): accretion, accretion disks - black hole physics - Galaxy: center - radiation mechanisms: general

CDS comments: Star S2 = [GKM98] S0-2

Simbad objects: 4

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Number of rows : 4

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
#notes
1 GCIRS 16 Cl* 17 45 40.0 -29 00 28           ~ 316 0
2 NAME Sgr A* X 17 45 40.03599 -29 00 28.1699           ~ 3597 3
3 NAME Gal Center reg 17 45 40.04 -29 00 28.1           ~ 11996 0
4 [EG97] S2 * 17 45 40.0442 -29 00 27.975           B0/2V 293 1

    Equat.    Gal    SGal    Ecl

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2021.03.01-09:25:52

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