Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR1.2k papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR954 papers
- University of CambridgeGB949 papers
- Universitat de ValènciaES937 papers
- University of ManchesterGB903 papers
- University of MilanIT896 papers
- University of ChicagoUS883 papers
- Radboud University NijmegenNL879 papers
- Sapienza University of RomeIT879 papers
- University College LondonGB874 papers
- University of OxfordGB873 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR868 papers
18 papers · 2 filters
CO-CAVITY pilot survey: Molecular gas and star formation in void galaxies
J. Domínguez-Gómez, U. Lisenfeld, I. Pérez +9
We present the first molecular gas mass survey of void galaxies. We compare these new data together with data for the atomic gas mass and star formation rate () from the l…
Revealing the structure of the lensed quasar Q 0957+561: I. Accretion disk size
C. Fian, E. Mediavilla, J. Jiménez-Vicente +6
We aim to use signatures of microlensing induced by stars in the foreground lens galaxy to infer the size of the accretion disk in the gravitationally lensed quasar Q 0957+561. The…
Local variations of the Stellar Velocity Ellipsoid-I: the disc of galaxies in the Auriga simulations
Daniel Walo-Martín, Isabel Pérez, Robert J. J. Grand +3
The connection between the Stellar Velocity Ellipsoid (SVE) and the dynamical evolution of galaxies has been a matter of debate in the last years and there is no clear consensus wh…
Revealing the structure of the lensed quasar Q 0957+561: III. SMBH mass via gravitational redshift
C. Fian, E. Mediavilla, J. Jiménez-Vicente +4
We intend to use the impact of microlensing on the Fe III emission line blend along with a measure of its gravitational redshift to estimate the mass of the quasar's central superm…
Microlensing of the broad emission lines in 27 gravitationally lensed quasars. Broad line region structure and kinematics
C. Fian, E. Mediavilla, V. Motta +4
We aim to study the structure and kinematics of the broad line region (BLR) of a sample of 27 gravitationally lensed quasars with up to five different epochs of observation. This s…
NOEMA Observations of CO Emission in Arp 142 and Arp 238
Cong K. Xu, Ute Lisenfeld, Yu Gao +1
Previous studies have shown significant differences in the enhancement of the star-formation rate (SFR) and the star-formation efficiency (SFE=SFR/M_mol) between spiral-spiral and…
Detecting hot stars in the Galactic centre with combined near- and mid-infrared photometry
M. Cano-González, R. Schödel, F. Nogueras-Lara
{The Galactic centre (GC) is a unique astrophysical laboratory to study the stellar population of galactic nuclei because it is the only galactic nucleus whose stars can be resolve…
ALMA Lensing Cluster Survey: A spectral stacking analysis of [CII] in lensed galaxies
Jean-Baptiste Jolly, Kirsten Knudsen, Nicolas Laporte +14
The properties of galaxies at redshift hold the key to our understanding of the early stages of galaxy evolution and can potentially identify the sources of the ultraviolet r…
Molecular gas and star formation within 12 strong galactic bars observed with IRAM-30m
Simón Díaz-García, Ute Lisenfeld, Isabel Pérez +8
While some galactic bars show recent massive star formation (SF) along them, some others present a lack of it. Whether bars with low level of SF are a consequence of low star forma…
Are all post-starbursts mergers? HST reveals hidden disturbances in the majority of PSBs
Elizaveta Sazonova, Katherine Alatalo, Kate Rowlands +12
How do galaxies transform from blue, star-forming spirals to red, quiescent early-type galaxies? To answer this question, we analyzed a set of 26 gas-rich, shocked post-starburst g…
Physical Characterization of Serendipitously Uncovered Millimeter-wave Line-emitting Galaxies at z~2.5 behind the Local Luminous Infrared Galaxy VV114
S. Mizukoshi, K. Kohno, F. Egusa +11
We present a detailed investigation of millimeter-wave line emitters ALMA J010748.3-173028 (ALMA-J0107a) and ALMA J010747.0-173010 (ALMA-J0107b), which were serendipitously uncover…
Detection of metallicity correlations in 100 nearby galaxies
Zefeng Li, Mark R. Krumholz, Emily Wisnioski +4
In this paper we analyse the statistics of the 2D gas-phase oxygen abundance distributions of 100 nearby galaxies drawn from the Calar Alto Legacy Integral Field spectroscopy Area…
A Giant Molecular Cloud Catalog in the Molecular Disk of the Elliptical Galaxy NGC 5128 (Centaurus A)
E. R. Miura, D. Espada, A. Hirota +17
We present the first census of giant molecular clouds (GMCs) complete down to 10 and within the inner 4 kpc of the nearest giant elliptical and powerful radio galaxy,…
Isocyanic acid (HNCO) in the Hot Molecular Core G331.512-0.103: Observations and Chemical Modelling
Carla M. Canelo, Leonardo Bronfman, Edgar Mendoza +5
Isocyanic acid (HNCO) is a simple molecule with a potential to form prebiotic and complex organic species. Using a spectral survey collected with the Atacama Pathfinder EXperiment…
The origin of bulges and discs in the CALIFA survey: I. Morphological evolution
J. Mendez-Abreu, A. de Lorenzo-Caceres, S. F. Sanchez
This series of papers aims at understanding the formation and evolution of non-barred disc galaxies. We use the new spectro-photometric decomposition code, C2D, to separate the spe…
Morphological and Kinematical Analysis of the Double-barred Galaxy NGC 3504 Using ALMA CO (2-1) Data
Yu-Ting Wu, Alfonso Trejo, Daniel Espada +1
We present results obtained from ALMA CO (2-1) data of the double-barred galaxy NGC 3504. With three times higher angular resolution (~ 0."8) than previous studies, our observation…
A duality in the origin of bulges and spheroidal galaxies
L. Costantin, P. G. Pérez-González, J. Méndez-Abreu +11
Studying the resolved stellar populations of the different structural components which build massive galaxies directly unveils their assembly history. We aim at characterizing the…
J-PLUS: The star formation main sequence and rate density at d < 75 Mpc
G. Vilella-Rojo, R. Logroño-García, C. López-Sanjuan +20
Our goal is to estimate the star formation main sequence (SFMS) and the star formation rate density (SFRD) at z <= 0.017 (d < 75 Mpc) using the Javalambre Photometric Local Univers…