Zobrazeno 1 - 10
of 18
pro vyhledávání: '"E. O. Schmidt"'
NGC 4945 harbors one of the nearest active galactic nuclei (AGN), which allows reaching high spatial resolution with the current observational facilities. The Seyfert 2 nucleus is deeply obscured by an edge-on disk with $A_V\sim14$, requiring infrare
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d028566a9f071027936f848a1baf030d
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
In order to study the slope and strength of the non-stellar continuum, we analyzed a sample of nearby Narrow Line Seyfert 1 (NLS1). Also, we re-examined the location of NLS1 galaxies on the M $-$ $\sigma$ relation using the stellar velocity dispersio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1efc6b214eeda139f793e319efb8160d
http://arxiv.org/abs/1906.07909
http://arxiv.org/abs/1906.07909
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
In order to study the location of circumnuclear rings (CNR) and their possible relation with the inner Lindblad resonances (ILR), we investigate a sample of spiral galaxies. For this purpose, we have obtained and analyzed medium resolution spectra of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::82d2fe6a546788611f725b1fb6224e73
http://arxiv.org/abs/1906.04843
http://arxiv.org/abs/1906.04843
Autor:
M. G. Volpe, L. A. Gutiérrez-Soto, E. O. Schmidt, Roberto Claudio Gamen, W. A. Weidmann, Damian Mast, G. Gaspar, G. A. Oio, M. M. Miller Bertolami, M. B. Mari
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Planetary nebulae represent a potential late stage of stellar evolution, however the central stars (CSPNe) are relatively faint and therefore pertinent information is merely available for
Accepted to be published in the A&A
Accepted to be published in the A&A
Autor:
C. Fariña, I. Ordonez-Etxeberria, E. O. Schmidt, W. A. Weidmann, Roberto Claudio Gamen, Damian Mast, Richard Ashley, L. Peralta de Arriba, G. Gimeno, P. Sowicka
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP
Context. There are more than 3000 known Galactic planetary nebulae (PNe), but only 492 central stars of Galactic planetary nebulae (CSPN) have known spectral types. It is vital to increase this number in order to have reliable statistics, which will
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c98525271baf75b425e0c1ff5305bfcd
http://arxiv.org/abs/1802.02122
http://arxiv.org/abs/1802.02122
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Many active galactic nuclei (AGN) and particularly narrow-line Seyfert 1 (NLS1) galaxies, usually exhibit blueshifts and blue wings in several emission lines, which are mainly associated with outflows and strong winds. In order to study the radial ve
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f574786dc2560d8362c9740c89681c14
https://www.aanda.org/10.1051/0004-6361/201731557
https://www.aanda.org/10.1051/0004-6361/201731557
Autor:
R. R. Vena Valdarenas, E. O. Schmidt, Walter Alfredo Weidmann, J. A. Ahumada, A. Mudrik, M. G. Volpe
We present an atlas of more than one hundred original images of planetary nebulae (PNe). These images were taken in a narrow-band filter centred on the nebular emission of the [N II] during several observing campaigns using two moderate-aperture tele
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::029656aff4ecde50a6e06f50954ca03b
http://arxiv.org/abs/1606.01066
http://arxiv.org/abs/1606.01066
Autor:
Maria Victoria Alonso, D. García Lambas, Georgina Coldwell, G. A. Oio, L. Donoso, E. O. Schmidt
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
The main goal of this study was to determine the effects on equivalent widths (EWs) of some spectral lines produced in the quasars by the presence of surrounding galaxies. To carry this out, a sample of 4663 quasars (QSOs) in the redshift range of 0.
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
It is not yet well known whether narrow line Seyfert 1 (NLS1) galaxies follow the $M_{BH} - \sigma_{\star}$ relation found for normal galaxies. Emission lines, such as [SII] or [OIII]$\lambda$5007, have been used as a surrogate of the stellar velocit
Publikováno v:
Journal of Applied Meteorology. 34:447-459
Brightness temperature difference (BTD) values are calculated for selected Geostationary Operational Environmental Satellite (GOES-6) channels (3.9, 12.7 µm) and Advanced Very High Resolution Radiometer channels (3.7, 12.0 µm). Daytime and nighttim