Search Publications

Properties of IR-selected active galactic nuclei
DOI: 10.1051/0004-6361/202142228 Bibcode: 2022A&A...664A.110B

García Lambas, D.; Alonso, M. V.; Bornancini, C. G. +1 more

Context. Active galactic nuclei (AGNs) of galaxies play an important role in the life and evolution of galaxies through the impact they exert on certain properties and on the evolutionary path of galaxies. It is well known that infrared (IR) emission is useful for selecting galaxies with AGNs, although it has been observed that there is contaminat…

2022 Astronomy and Astrophysics
eHST 4
The Cluster Ages Experiment (CASE) - IX. Analysis of four detached eclipsing binaries in the globular cluster NGC 3201
DOI: 10.1093/mnras/stac2751 Bibcode: 2022MNRAS.517.2485R

Marshall, J. L.; Thompson, I. B.; Morrell, N. +14 more

We use photometric and spectroscopic observations of four detached eclipsing binaries in the globular cluster NGC 3201 to derive masses, radii, and luminosities of the component stars. Spanning across almost three magnitudes in the colour-magnitude diagram, the components offer a unique possibility to test the theory of stellar evolution. Their ma…

2022 Monthly Notices of the Royal Astronomical Society
Gaia eHST 4
Detached eclipsing binaries from the Kepler field: radii and photometric masses of components in short-period systems
DOI: 10.1093/mnras/stac1707 Bibcode: 2022MNRAS.515.1416C

Diaz, Marcos P.; Cruz, Patricia; Aguilar, John F. +2 more

The characterization of detached eclipsing binaries with low-mass components has become important when verifying the role of convection in stellar evolutionary models, which requires model-independent measurements of stellar parameters with great precision. However, spectroscopic characterization depends on single-target radial velocity observatio…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 4
VLA Observations of the AE Aqr-type Cataclysmic Variable LAMOST J024048.51+195226.9
DOI: 10.3847/1538-3881/ac3ed9 Bibcode: 2022AJ....163...58B

Barrett, Paul E.

AE Aqr was until recently the only known magnetic cataclysmic variable (MCV) containing a rapidly spinning (33.08 s) white dwarf (WD). Its radio emission is believed to be a superposition of synchrotron-emitting plasmoids, because it has a positive spectral index spanning three orders of magnitude (≈2-2000 GHz) and is unpolarized. Both characteris…

2022 The Astronomical Journal
Gaia 4
On the synergy between Ariel and ground-based high-resolution spectroscopy
DOI: 10.1007/s10686-021-09824-7 Bibcode: 2022ExA....53..655G

Sozzetti, Alessandro; Bonomo, Aldo S.; Guilluy, Gloria +2 more

Since the first discovery of an extra-solar planet around a main-sequence star, in 1995, the number of detected exoplanets has increased enormously. Over the past two decades, observational instruments (both onboard and on ground-based facilities) have revealed an astonishing diversity in planetary physical features (i. e. mass and radius), and or…

2022 Experimental Astronomy
eHST 4
Water ortho-to-para ratio in the coma of comet 67P/Churyumov-Gerasimenko
DOI: 10.1051/0004-6361/202142494 Bibcode: 2022A&A...663A..43C

Encrenaz, T.; Erard, S.; Crovisier, J. +9 more

Context. Abundance ratios of the nuclear-spin isomers of H2O and NH3 have been measured in about two dozen comets, with a mean value corresponding to a nuclear-spin temperature of ~30 K. The real meaning of these unequilibrated nuclear-spin abundance ratios is still debated. However, an equilibrated water ortho-to-para ratio …

2022 Astronomy and Astrophysics
Rosetta 4
The Distribution of UV Radiation Field in the Molecular Clouds of Gould Belt
DOI: 10.1088/1674-4527/ac784e Bibcode: 2022RAA....22h5017X

Li, Di; Xie, Jinjin; Fuller, Gary A. +5 more

The distribution of ultraviolet (UV) radiation field provides critical constraints on the physical environments of molecular clouds. Within 1 kpc of our solar system and fostering protostars of different masses, the giant molecular clouds in the Gould Belt present an excellent opportunity to resolve the UV field structure in star-forming regions. …

2022 Research in Astronomy and Astrophysics
Herschel 4
The galaxy population of the core of the Coma cluster
DOI: 10.1093/mnras/stab3427 Bibcode: 2022MNRAS.510.4463P

Hasan, S. N.; Poloji, Nagamani; Hasan, Priya

In this paper, we present the structural properties and morphology of galaxies in the central region of the Coma Cluster brighter than 19.5 mag in the F814W band from the HST/ACS Coma Cluster Treasury Survey. Using mainly spectroscopic redshifts, we find 132 members from our sample of 219 galaxies. In our sample of 132 members, we find 51 non-dwar…

2022 Monthly Notices of the Royal Astronomical Society
eHST 4
Evolution of pits at the surface of 67P/Churyumov-Gerasimenko
DOI: 10.1051/0004-6361/202243983 Bibcode: 2022A&A...668A.132B

Guilbert-Lepoutre, Aurélie; Besse, Sébastien; Benseguane, Selma +6 more

Context. The observation of pits at the surface of comets offers the opportunity to take a glimpse into the properties and the mechanisms that shape a nucleus through cometary activity. If the origin of these pits is still a matter of debate, multiple studies have recently suggested that known phase transitions (such as volatile sublimation or amo…

2022 Astronomy and Astrophysics
Rosetta 4
Seismic modelling of the pulsating mercury-manganese star HD 29589
DOI: 10.1093/mnras/stac1632 Bibcode: 2022MNRAS.514.5640N

Niemczura, E.; Hubrig, S.; Hummel, C. A. +4 more

Photometric and spectroscopic time-series of chemically peculiar mercury-manganese (HgMn) stars show variability, which in most cases is interpreted as the effect of binarity or surface spots. Until recently, pulsations have not been detected in these objects. However, the analysis of the Transiting Exoplanet Survey Satellite (TESS) photometric ti…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 4