Zobrazeno 1 - 10
of 34
pro vyhledávání: '"Moser, Lydia"'
Autor:
Moser, Lydia, Sánchez-Monge, Álvaro, Eckart, Andreas, Requena-Torres, Miguel Angel, García-Marin, Macarena, Kunneriath, Devaky, Zensus, Anton, Britzen, Silke, Sabha, Nadeen, Shahzamanian, Banafsheh, Borkar, Abhijeet, Fischer, Sebastian
Publikováno v:
The Multi-Messenger Astrophysics of the Galactic Centre, Proceedings of the International Astronomical Union, IAU Symposium, 2017, Volume 322, pp. 129-132
We report serendipitous detections of line emission with ALMA in band 3, 6, and 7 in the central parsec of the Galactic center at an up to now highest resolution (<0.7''). Among the highlights are the very first and highly resolved images of sub-mm m
Externí odkaz:
http://arxiv.org/abs/1707.02951
Autor:
Moser, Lydia, Krips, Melanie, Busch, Gerold, Scharwaechter, Julia, Koenig, Sabine, Eckart, Andreas, Smajic, Semir, Garcia-Marin, Macarena, Valencia-S., Monica, Fischer, Sebastian, Dierkes, Jens
Publikováno v:
Astronomy & Astrophysics, Volume 587, March 2016, id.A137, 21 pp
We present a pilot study of ~ 3" resolution observations of low CO transitions with the Submillimeter Array in three nearby Seyfert galaxies, which are part of the low-luminosity quasi-stellar object (LLQSOs) sample consisting of 99 nearby (z = 0.06)
Externí odkaz:
http://arxiv.org/abs/1707.01081
Autor:
Moser, Lydia, Sánchez-Monge, Álvaro, Eckart, Andreas, Requena-Torres, Miguel Angel, García-Marin, Macarena, Kunneriath, Devaky, Zensus, Anton, Britzen, Silke, Sabha, Nadeen, Shahzamanian, Banafsheh, Borkar, Abhijeet, Fischer, Sebastian
Publikováno v:
A&A 603, A68 (2017)
We report serendipitous detections of line emission with the Atacama Large Millimeter/submillimeter Array (ALMA) in band 3, 6, and 7 in the central parsec down to within 1" around Sgr A* at an up to now highest resolution (<0.5") view of the Galactic
Externí odkaz:
http://arxiv.org/abs/1603.00801
Autor:
Busch, Gerold, Fazeli, Nastaran, Smajić, Semir, Eckart, Andreas, Moser, Lydia, Valencia-S., Mónica
Integral-field spectroscopy in the near-infrared (NIR) is a powerful tool to analyze the gaseous and stellar distributions and kinematics, as well as the excitation mechanisms in the centers of galaxies. The unique combination of NIR and sub-mm data
Externí odkaz:
http://arxiv.org/abs/1511.03151
Autor:
Busch, Gerold, Fazeli, Nastaran, Eckart, Andreas, Valencia-S., Mónica, Smajić, Semir, Moser, Lydia, Scharwächter, Julia, Dierkes, Jens, Fischer, Sebastian
Publikováno v:
A&A 587, A138 (2016)
We present near-infrared (NIR) $H+K$-band longslit spectra of eleven galaxies which are obtained with SOFI at the NTT (ESO). The galaxies are chosen from the low-luminosity type-1 quasi-stellar object (LLQSO) sample which comprises the 99 closest ($z
Externí odkaz:
http://arxiv.org/abs/1511.00904
Autor:
Busch, Gerold, Smajić, Semir, Scharwächter, Julia, Eckart, Andreas, Valencia-S., Mónica, Moser, Lydia, Husemann, Bernd, Krips, Melanie, Zuther, Jens
Publikováno v:
A&A 575, A128 (2015)
Circumnuclear star formation and AGN feedback is believed to play a critical role in the context of galaxy evolution. The low-luminosity QSO (LLQSO) sample that contains 99 of the closest AGN with redshift z<=0.06 fills the gap between the local AGN
Externí odkaz:
http://arxiv.org/abs/1412.2069
Autor:
Smajic, Semir, Moser, Lydia, Eckart, Andreas, Valencia-S., Monica, Combes, Francoise, Horrobin, Matthew, Garcia-Burillo, Santiago, Garcia-Marin, Macarena, Fischer, Sebastian, Zuther, Jens
Publikováno v:
A&A 567, A119 (2014)
We present the results of near-infrared (NIR) H- and K-band European Southern Observatory SINFONI integral field spectroscopy (IFS) of the Seyfert 2 galaxy NGC 1433. We present emission and absorption line measurements in the central kpc of NGC 1433.
Externí odkaz:
http://arxiv.org/abs/1404.6562
Autor:
Busch, Gerold, Zuther, Jens, Valencia-S., Mónica, Moser, Lydia, Fischer, Sebastian, Eckart, Andreas, Scharwächter, Julia, Gadotti, Dimitri A., Wisotzki, Lutz
Recognizing the properties of the host galaxies of quasi-stellar objects (QSOs) is essential to understand the suspected coevolution of central supermassive black holes (BHs) and their host galaxies. We selected a subsample of the Hamburg/ESO survey
Externí odkaz:
http://arxiv.org/abs/1310.0272
Autor:
Moser, Lydia, Zuther, Jens, Fischer, Sebastian, Busch, Gerold, Valencia-S., Monica, Eckart, Andreas, Krips, Melanie, Scharwaechter, Julia
The low luminosity QSO (LLQSO) sample consists of type 1 active galactic nuclei (AGN) up to a redshift of z=0.06 in the Hamburg/ESO QSO survey. Its purpose is to study how the brightest AGN in the nearby universe evolve with respect to AGN activity a
Externí odkaz:
http://arxiv.org/abs/1309.6921
There is growing evidence that every galaxy with a considerable spheroidal component hosts a supermassive black hole (SMBH) at its center. Strong correlations between the SMBH and the spheroidal component suggest a physical connection through a coevo
Externí odkaz:
http://arxiv.org/abs/1307.1049