Zobrazeno 1 - 10
of 24
pro vyhledávání: '"Lakićević, Maša"'
Autor:
Lakicevic, Masa
This thesis presents the first population study of supernova remnants (SNRs) in one whole galaxy – the Large Magellanic Cloud (LMC) on submm and FIR wavelengths. The first part is about the dust production in supernovae (SNe) and SNRs, based on sev
Externí odkaz:
http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.695601
Publikováno v:
A&A 679, A34 (2023)
We explore the influence of optical Fe II quasi-continuum on the measured spectral parameters in the 4150-5500 A range for the spectra of Type 1 active galactic nuclei (AGNs). We assume that the broad line region is composed of two sub-regions: the v
Externí odkaz:
http://arxiv.org/abs/2309.14852
Autor:
Kovacevic, Andjelka B., Radovic, Viktor, Ilic, Dragana, Popovic, Luka C., Assef, Roberto J., Sanchez-Saez, Paula, Nikutta, Robert, Raiteri, Claudia M., Yoon, Ilsang, Homayouni, Yasaman, Li, Yan-Rong, Caplar, Neven, Czerny, Bozena, Panda, Swayamtrupta, Ricci, Claudio, Jankov, Isidora, Landt, Hermine, Wolf, Christian, Kovacevic-Dojcinovic, Jelena, Lakicevic, Masa, Savic, Djorđe, Vince, Oliver, Simic, Sasa, Cvorovic-Hajdinjak, Iva, Marceta-Mandic, Sladjana
The Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) will detect an unprecedentedly large sample of actively accreting supermassive black holes with typical accretion disk (AD) sizes of a few light days. This brings us to face challen
Externí odkaz:
http://arxiv.org/abs/2208.06203
Publikováno v:
A&A 659, A130 (2022)
We have used the sample of 577 active galactic nuclei Type 1.8-2 spectra (z < 0.25), taken from Sloan Digital Sky Survey, to trace the influence of the outflow kinematics to the profiles of different emission lines (Hbeta, [O III], Halpha, [N II], [S
Externí odkaz:
http://arxiv.org/abs/2112.11797
The differences between Narrow Line Seyfert 1 galaxies (NLS1s) and Broad Line AGNs (BLAGNs) are not completely understood; it is thought that they may have different inclinations and/or physical characteristics. The FWHM(Hb)-luminosities correlations
Externí odkaz:
http://arxiv.org/abs/2110.06687
We investigated narrow line Seyfert 1 galaxies (NLS1s) at optical, mid-infrared (MIR) and X-ray wavelengths, comparing them to the broad line active galactic nuclei (BLAGNs). We found that black hole mass, coronal line luminosities, X-ray hardness ra
Externí odkaz:
http://arxiv.org/abs/1805.06437
The optical vs. mid-infrared spectral properties of 82 Type 1 AGNs: coevolution of AGN and starburst
We investigated the connection between the mid-infrared (MIR) and optical spectral characteristics in a sample of 82 Type 1 active galactic nuclei (AGNs), observed with Infrared Spectrometer on Spitzer (IRS) and Sloan Digital Sky Survey (SDSS, DR12).
Externí odkaz:
http://arxiv.org/abs/1707.08395
Autor:
Lakićević, Maša, van Loon, Jacco Th., Meixner, Margaret, Gordon, Karl, Bot, Caroline, Roman-Duval, Julia, Babler, Brian, Bolatto, Alberto, Engelbracht, Chad, Filipović, Miroslav, Hony, Sacha, Indebetouw, Remy, Misselt, Karl, Montiel, Edward, Okumura, K., Panuzzo, Pasquale, Patat, Ferdinando, Sauvage, Marc, Seale, Jonathan, Sonneborn, George, Temim, Tea, Urošević, Dejan, Zanardo, Giovanna
We present the analysis of supernova remnants (SNRs) in the Large Magellanic Cloud (LMC) and their influence on the environment at far-infrared (FIR) and submillimeter wavelengths. We use new observations obtained with the {\it Herschel} Space Observ
Externí odkaz:
http://arxiv.org/abs/1410.5709
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.