Search Publications

A Deep View into the Nucleus of the Sagittarius Dwarf Spheroidal Galaxy with MUSE. III. Discrete Multicomponent Population-dynamical Models Based on the Jeans Equations
DOI: 10.3847/1538-4357/ac9280 Bibcode: 2022ApJ...939..118K

Lützgendorf, Nora; Böker, Torsten; Kamann, Sebastian +12 more

We present comprehensive multicomponent dynamical models of M54 (NGC 6715), the nuclear star cluster of the Sagittarius (Sgr) dwarf galaxy, which is undergoing a tidal disruption in the Milky Way halo. Previous papers in this series used a large MUSE mosaic data set to identify multiple stellar populations in the system and study their kinematic d…

2022 The Astrophysical Journal
eHST 13
OCCASO. IV. Radial velocities and open cluster kinematics
DOI: 10.1051/0004-6361/202141832 Bibcode: 2022A&A...658A..14C

Jordi, C.; Casamiquela, L.; Cantat-Gaudin, T. +8 more

Context. Open clusters (OCs) are widely used as test particles to investigate a variety of astrophysical phenomena, from stellar evolution to Galactic evolution. Gaia and the complementary massive spectroscopic surveys are providing an unprecedented wealth of information about these systems.
Aims: The Open Cluster Chemical Abundances from Spa…

2022 Astronomy and Astrophysics
Gaia 13
Assessing the role of clay and salts on the origin of MARSIS basal bright reflections
DOI: 10.1016/j.epsl.2022.117370 Bibcode: 2022E&PSL.57917370M

Orosei, Roberto; Caprarelli, Graziella; Pettinelli, Elena +7 more

Anomalously bright basal reflections detected by MARSIS at Ultimi Scopuli have been interpreted to indicate the presence of water-saturated materials or ponded liquid water at the base of the South Polar Layered Deposits (SPLD). Because conventional models assume basal temperatures (≤200 K) much lower than the melting point of water, this interpre…

2022 Earth and Planetary Science Letters
MEx 13
Validation scheme for solar coronal models: Constraints from multi-perspective observations in EUV and white light
DOI: 10.1051/0004-6361/202141552 Bibcode: 2022A&A...657A.117W

Temmer, M.; Asvestari, E.; Pomoell, J. +2 more

Context. In this paper, we present a validation scheme to investigate the quality of coronal magnetic field models, which is based on comparisons with observational data from multiple sources.
Aims: Many of these coronal models may use a range of initial parameters that produce a large number of physically reasonable field configurations. How…

2022 Astronomy and Astrophysics
SOHO 13
SPYGLASS. II. The Multigenerational and Multiorigin Star Formation History of Cepheus Far North
DOI: 10.3847/1538-4357/ac9b45 Bibcode: 2022ApJ...941...49K

Murphy, Simon J.; Rizzuto, Aaron C.; Kraus, Adam L. +4 more

Young stellar populations provide a record of past star formation, and by establishing their members' dynamics and ages, it is possible to reconstruct the full history of star formation events. Gaia has greatly expanded the number of accessible stellar populations, with one of the most notable recently discovered associations being Cepheus Far Nor…

2022 The Astrophysical Journal
Gaia 13
A Multiwavelength Study of GRS 1716-249 in Outburst: Constraints on Its System Parameters
DOI: 10.3847/1538-4357/ac6ce1 Bibcode: 2022ApJ...932...38S

Soria, Roberto; Gandhi, Poshak; Homan, Jeroen +27 more

We present a detailed study of the evolution of the Galactic black hole transient GRS 1716-249 during its 2016-2017 outburst at optical (Las Cumbres Observatory), mid-infrared (Very Large Telescope), near-infrared (Rapid Eye Mount telescope), and ultraviolet (the Neil Gehrels Swift Observatory Ultraviolet/Optical Telescope) wavelengths, along with…

2022 The Astrophysical Journal
Gaia 13
Identification, mass, and age of primary red clump stars from spectral features derived with the LAMOST DR7
DOI: 10.1093/mnras/stac484 Bibcode: 2022MNRAS.512.1710H

Luo, A. -Li; Chen, Yu-Qin; He, Xu-Jiang

Although red clump (RC) stars are easy to identify due to their stability of luminosity and colour, about 20-50 per cent are actually red giant branch (RGB) stars in the same location on the HR diagram. In this paper, a sample of 210 504 spectra for 184 318 primary RC (PRC) stars from the LAMOST DR7 is identified, which has a purity of higher than…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 13
10 Yr Transformation of the Obscuring Wind in NGC 5548
DOI: 10.3847/2041-8213/ac822f Bibcode: 2022ApJ...934L..24M

Gu, Liyi; Kriss, Gerard A.; Mehdipour, Missagh +4 more

A decade ago, the archetypal Seyfert-1 galaxy NGC 5548 was discovered to have undergone major spectral changes. The soft X-ray flux had dropped by a factor of 30 while new broad and blueshifted UV absorption lines appeared. This was explained by the emergence of a new obscuring wind from the accretion disk. Here we report on the striking long-term…

2022 The Astrophysical Journal
eHST 13
MUSE sneaks a peek at extreme ram-pressure stripping events - V. Towards a complete view of the galaxy cluster A1367
DOI: 10.1093/mnras/stac345 Bibcode: 2022MNRAS.511.5180P

Fumagalli, Michele; Yoshida, Michitoshi; Fossati, Matteo +6 more

We present an analysis of the kinematics and ionization conditions in a sample composed of seven star-forming galaxies undergoing ram-pressure stripping in the A1367 cluster, and the galaxy ESO137-001 in the Norma cluster. MUSE observations of two new galaxies in this sample, CGCG097-073 and CGCG097-079, are also presented. This sample is characte…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 13
J-PLUS: a catalogue of globular cluster candidates around the M 81/M 82/NGC 3077 triplet of galaxies
DOI: 10.1093/mnras/stac2002 Bibcode: 2022MNRAS.516.1320C

Chies-Santos, Ana L.; Cenarro, A. Javier; Dupke, Renato +16 more

Globular clusters (GCs) are proxies of the formation assemblies of their host galaxies. However, few studies exist targeting GC systems of spiral galaxies up to several effective radii. Through 12-band Javalambre Photometric Local Universe Survey (J-PLUS) imaging, we study the point sources around the M 81/M 82/NGC 3077 triplet in search of new GC…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 13