Millimeter to X-ray flares from Sagittarius A*

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F12%3A00371579" target="_blank" >RIV/67985815:_____/12:00371579 - isvavai.cz</a>

Result on the web

<a href="http://dx.doi.org/10.1051/0004-6361/201117779" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201117779</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1051/0004-6361/201117779" target="_blank" >10.1051/0004-6361/201117779</a>

Result language

angličtina

Original language name

Millimeter to X-ray flares from Sagittarius A*

Original language description

We study the applicability of the adiabatic synchrotron source expansion model and study physical processes giving rise to the variable emission of SgrA* from the radio to the X-ray domain. Our observations were carried out on 18 May 2009 using the NACOadaptive optics (AO) instrument at the European Southern Observatory's Very Large Telescope, the ACIS-I instrument aboard the Chandra X-ray Observatory, the LABOCA bolometer at the Atacama Pathfinder EXperiment (APEX), and the CARMA mm telescope array atCedar Flat, California.

Czech name

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Czech description

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Type

J_x - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

CEP classification

BN - Astronomy and celestial mechanics, astrophysics

OECD FORD branch

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Project

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Continuities

Z - Vyzkumny zamer (s odkazem do CEZ)

Publication year

2012

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Name of the periodical

Astronomy & Astrophysics

ISSN

0004-6361

e-ISSN

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Volume of the periodical

537

Issue of the periodical within the volume

January

Country of publishing house

FR - FRANCE

Number of pages

18

Pages from-to

"A52/1"-"A52/18"

UT code for WoS article

000300416800052

EID of the result in the Scopus database

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