Activity of the mass-accreting compact objects - prospects for the optical monitoring

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21230%2F12%3A00225292" target="_blank" >RIV/68407700:21230/12:00225292 - isvavai.cz</a>

Výsledek na webu

<a href="http://astron-soc.in/bulletin/asics_vol007/287-Simon.pdf" target="_blank" >http://astron-soc.in/bulletin/asics_vol007/287-Simon.pdf</a>

DOI - Digital Object Identifier

—

Jazyk výsledku

angličtina

Název v původním jazyce

Activity of the mass-accreting compact objects - prospects for the optical monitoring

Popis výsledku v původním jazyce

We discuss the perspectives of investigation of the mass-accreting compact objects in the binary systems, for example cataclysmic variables (CVs), with monitors. Especially the processes that operate on timescales of years are little studied, hence little understood. However, the profiles of the light curves can be significantly affected by the sampling of data from the monitors. We show an approximation of how the profiles of these light curves change after a heavy sampling of the data. We find that histograms of brightness (in magnitudes) provide us with a representative description of the properties of the long-term activity of a given type of CV even in the sampled data. We also discuss the strategy of monitoring of these systems, particularly as regards the spatial distribution of these systems in the Galaxy and their peak brightness.

Název v anglickém jazyce

Activity of the mass-accreting compact objects - prospects for the optical monitoring

Popis výsledku anglicky

We discuss the perspectives of investigation of the mass-accreting compact objects in the binary systems, for example cataclysmic variables (CVs), with monitors. Especially the processes that operate on timescales of years are little studied, hence little understood. However, the profiles of the light curves can be significantly affected by the sampling of data from the monitors. We show an approximation of how the profiles of these light curves change after a heavy sampling of the data. We find that histograms of brightness (in magnitudes) provide us with a representative description of the properties of the long-term activity of a given type of CV even in the sampled data. We also discuss the strategy of monitoring of these systems, particularly as regards the spatial distribution of these systems in the Galaxy and their peak brightness.

Druh

D - Stať ve sborníku

CEP obor

JA - Elektronika a optoelektronika, elektrotechnika

OECD FORD obor

—

Projekt

<a href="/cs/project/GA102%2F09%2F0997" target="_blank" >GA102/09/0997: Automatická detekce a obrazová analýza optické emise kosmických gama záblesků</a><br>

Návaznosti

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Rok uplatnění

2012

Kód důvěrnosti údajů

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

Název statě ve sborníku

Second Workshop on Robotic Autonomous Observatories

ISBN

978-81-922926-5-6

ISSN

—

e-ISSN

—

Počet stran výsledku

9

Strana od-do

287-295

Název nakladatele

Astronomical Society of India

Místo vydání

Bengaluru

Místo konání akce

Torremolinos-Malaga

Datum konání akce

5. 6. 2011

Typ akce podle státní příslušnosti

WRD - Celosvětová akce

Kód UT WoS článku

—