2009A&A...505..169B

Query : 2009A&A...505..169B

2009A&A...505..169B - Astronomy and Astrophysics, volume 505, 169-176 (2009/10-1)

Cosmic ray acceleration parameters from multi-wavelength observations. The case of SN 1006.

BEREZHKO E.G., KSENOFONTOV L.T. and VOELK H.J.

Abstract (from CDS):

The properties of the Galactic supernova remnant (SNR) SN 1006 are theoretically reanalysed. Nonlinear kinetic theory is used to determine the acceleration efficiency of cosmic rays (CRs) in the supernova remnant SN 1006. The known range of astronomical parameters and the existing measurements of nonthermal emission are examined in order to define the values of the relevant physical parameters that determine the CR acceleration efficiency. It is shown that the parameter values - proton injection rate, electron to proton ratio and downstream magnetic field strength -are determined with the appropriate accuracy. In particular the observed azimuthal variations in the γ-ray morphology also agree with the theoretical expectation. These parameter values, together with the reduction of the γ-ray flux relative to a spherically symmetric acceleration geometry, allow a good fit to the existing data, including the recently detected TeV emission by H.E.S.S. SN 1006 represents the first example where a high efficiency of nuclear CR production, required for the Galactic CR sources, is consistently established.

Abstract Copyright: ∼

Journal keyword(s): ISM: cosmic rays - acceleration of particles - shock waves - stars: supernovae: individual: SN 1006 - radiation mechanisms: nonthermal - gamma rays: theory

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 - 2023	#notes
1	NAME Lupus SN	SNR	15 02 22.1	-42 05 49						~	1298	1

Query : 2009A&A...505..169B

Basic data :

NAME Lupus SN -- SuperNova Remnant
Origin of the objects types : (Ref) Object type as listed in the reference "Ref" (acronym) Object type linked to the acronym according to the original reference () Anterior to 2007, before we can link the objet type to a reference, or given by the CDS team in some particular cases Other object types:	`X (1E,1ES,...)`, `SNR (2009BASI,AJG,...)`, `Rad (GRS,MRC,...)`, `SN* (SN)`, `gam (TeV)`
Syntax of coordinates is : "ra dec (wtype) [error ellipse] quality bibcode" : ra dec : right ascension and declination (unit and frame defined according to your Output Options) Grey values are increasing the original precision due to the computation of frame transformations (wtype) : wavelength class for the origin of the coordinates (Rad, mm, IR, Optical, UV, Xray, Gam) [error ellipse] : measurement uncertainty, on (ra,dec) if the positional angle is 90 degrees, on (majaxis,minaxis) otherwise (in mas at defined epoch in the original catalogue), position angle (in degrees North celestial pole to East) quality : flag of quality E ≥ 10" D : 1-10" (and some old data) C : 0.1-1" B : 0.01-0.1" + 2MASS, Tyc A : VLBI, Hipparcos bibcode : bibcode of the coordinates reference ICRS coord. (ep=J2000) :	`15 02 22.1 -42 05 49 [ 3000 3000 90 ] D 1990PKS...C......0W`
Syntax of coordinates is : "ra dec (wtype) [error ellipse] quality bibcode" : ra dec : right ascension and declination (unit and frame defined according to your Output Options) Grey values are increasing the original precision due to the computation of frame transformations (wtype) : wavelength class for the origin of the coordinates (Rad, mm, IR, Optical, UV, Xray, Gam) [error ellipse] : measurement uncertainty, on (ra,dec) if the positional angle is 90 degrees, on (majaxis,minaxis) otherwise (in mas at defined epoch in the original catalogue), position angle (in degrees North celestial pole to East) quality : flag of quality E ≥ 10" D : 1-10" (and some old data) C : 0.1-1" B : 0.01-0.1" + 2MASS, Tyc A : VLBI, Hipparcos bibcode : bibcode of the coordinates reference FK4 coord. (ep=B1950 eq=1950) :	`14 59 05.6 -41 54 02 [ 3000 3000 90 ]`
Syntax of coordinates is : "ra dec (wtype) [error ellipse] quality bibcode" : ra dec : right ascension and declination (unit and frame defined according to your Output Options) Grey values are increasing the original precision due to the computation of frame transformations (wtype) : wavelength class for the origin of the coordinates (Rad, mm, IR, Optical, UV, Xray, Gam) [error ellipse] : measurement uncertainty, on (ra,dec) if the positional angle is 90 degrees, on (majaxis,minaxis) otherwise (in mas at defined epoch in the original catalogue), position angle (in degrees North celestial pole to East) quality : flag of quality E ≥ 10" D : 1-10" (and some old data) C : 0.1-1" B : 0.01-0.1" + 2MASS, Tyc A : VLBI, Hipparcos bibcode : bibcode of the coordinates reference Gal coord. (ep=J2000) :	`327.4109 +14.4674 [ 3000 3000 90 ]`
Syntax of angular size is : "maj-axis min-axis angle (wtype) quality bibcode" maj-axis : major axis size (arc minutes) min-axis : minor axis size (arc minutes) angle : orientation angle (in degrees) (wtype) : wavelength class for the origin of the angular size (Rad, mm, IR, Opt, UV, Xray, Gam) quality : flag of quality of the angular size values ( A=best quality -> E=worst quality, {� } =unknown quality) bibcode : bibcode of the angular size reference Angular size (arcmin):	`30.0 30.0 90 (Rad) D` `2014BASI...42...47G`

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`NAME Lupus SN`	`H 1506-42`	`PKS 1459-419`	`SN 1006`
`AJG 37`	`KOHX 1`	`PKS J1502-4205`	`TeV J1502-419`
`1E 1459.6-4146`	`1M 1457-416`	`SNR G327.6+14.6`	`2U 1440-39`
`1ES 1500-41.5`	`MRC 1459-417`	`SNR G327.6+14.5`	`3U 1439-39`
`GRS G327.60 +14.60`	`MSH 14-4-15`	`SN 1006A`	`4U 1458-41`
`1H 1458-416`	`PKS 1459-41`	`SN 1016`	`XSS J15031-4149`

References (1298 between 1850 and 2023) (Total 1298)
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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Data at NED - NASA/IPAC Extragalactic Database : NAME Lupus SN

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PKS 1459-41 PKS 1459-419 PKS J1502-4205

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