Search Publications

Determining the parameters of the spiral arms of the Galaxy from kinematic tracers based on Gaia DR3 data
DOI: 10.1093/mnras/stad3350 Bibcode: 2024MNRAS.527.1472D

Akhmetov, V. S.; Fedorov, P. N.; Velichko, A. B. +2 more

We present the results of determining the parameters of the spiral arms of the Galaxy using the stars Gaia DR3, whose absolute magnitude is MG < 4, and which allow tracing spiral arms at large distances from the Sun. As tracers of spiral arms, we use the centroids of stellar spherical regions with a radius of 0.5 kpc, in which the de…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 6
The Extended [C II] under Construction? Observation of the Brightest High-z Lensed Star-forming Galaxy at z = 6.2
DOI: 10.3847/1538-4357/ad0f95 Bibcode: 2024ApJ...961...71F

Ravindranath, Swara; Mahler, Guillaume; Henry, Alaina +27 more

We present results of [C II] 158 µm emission line observations, and report the spectroscopic redshift confirmation of a strongly lensed (µ ~ 20) star-forming galaxy, MACS0308-zD1 at z = 6.2078 ± 0.0002. The [C II] emission line is detected with a signal-to-noise ratio >6 within the rest-frame UV-bright clump of the lensed galaxy (zD…

2024 The Astrophysical Journal
Gaia eHST 6
TESS Giants Transiting Giants. VI. Newly Discovered Hot Jupiters Provide Evidence for Efficient Obliquity Damping after the Main Sequence
DOI: 10.3847/1538-3881/ad543b Bibcode: 2024AJ....168...81S

Vanderburg, Andrew; Rice, Malena; Tan, Thiam-Guan +53 more

The degree of alignment between a star's spin axis and the orbital plane of its planets (the stellar obliquity) is related to interesting and poorly understood processes that occur during planet formation and evolution. Hot Jupiters orbiting hot stars (≳6250 K) display a wide range of obliquities, while similar planets orbiting cool stars are pref…

2024 The Astronomical Journal
Gaia 6
The TRAPUM Small Magellanic Cloud pulsar survey with MeerKAT - I. Discovery of seven new pulsars and two Pulsar Wind Nebula associations
DOI: 10.1093/mnras/stae1310 Bibcode: 2024MNRAS.531.2835C

Filipović, M. D.; Possenti, A.; Kramer, M. +17 more

The sensitivity of the MeerKAT radio interferometer is an opportunity to probe deeper into the population of rare and faint extragalactic pulsars. The TRAPUM (TRAnsients and PUlsars with MeerKAT) collaboration has conducted a radio-domain search for accelerated pulsars and transients in the Small Magellanic Cloud (SMC). This partially targeted sur…

2024 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 6
The First Catalog of Candidate White Dwarf–Main-sequence Binaries in Open Star Clusters: A New Window into Common Envelope Evolution
DOI: 10.3847/1538-4357/ad7500 Bibcode: 2024ApJ...976..102G

Drout, Maria R.; Muirhead, Philip S.; Speagle, Joshua S. +3 more

Close binary systems are the progenitors to both Type Ia supernovae and the compact object mergers that can be detected via gravitational waves. To achieve a binary with a small radial separation, it is believed that the system likely undergoes common envelope (CE) evolution. Despite its importance, CE evolution may be one of the largest uncertain…

2024 The Astrophysical Journal
Gaia 6
Assembling a high-precision abundance catalogue of solar twins in GALAH for phylogenetic studies
DOI: 10.1093/mnras/stae280 Bibcode: 2024MNRAS.529.2946W

Buder, Sven; Jofré, Paula; Aguilera-Gómez, Claudia +13 more

Stellar chemical abundances have proved themselves a key source of information for understanding the evolution of the Milky Way, and the scale of major stellar surveys such as GALAH have massively increased the amount of chemical data available. However, progress is hampered by the level of precision in chemical abundance data as well as the visua…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 6
The SRG/eROSITA All-Sky Survey: X-ray beacons at late cosmic dawn
DOI: 10.1051/0004-6361/202451035 Bibcode: 2024A&A...691A..30W

Salvato, M.; Buchner, J.; Nandra, K. +12 more

Context. The Spektrum-Roentgen-Gamma (SRG)/extended Roentgen Survey with an Imaging Telescope Array (eROSITA) All-Sky Survey (eRASS) is expected to contain ∼100 quasars that emitted their light when the universe was less than a billion years old, that is, at z > 5.6. By selection, these quasars populate the bright end of the active galactic nuc…

2024 Astronomy and Astrophysics
XMM-Newton 6
PHANGS Hubble Space Telescope Treasury Survey: Globular Cluster Systems in 17 Nearby Spiral Galaxies
DOI: 10.3847/1538-3881/ad1889 Bibcode: 2024AJ....167...95F

Leroy, Adam K.; Rosolowsky, Erik; Klessen, Ralf S. +18 more

We present new catalogs of likely globular clusters (GCs) in 17 nearby spiral galaxies studied as part of the PHANGS Hubble Space Telescope (HST) Treasury Survey. The galaxies were imaged in five broadband filters from the near-ultraviolet through the I band. PHANGS-HST has produced catalogs of stellar clusters of all ages by selecting extended so…

2024 The Astronomical Journal
Gaia eHST 6
Polycyclic Aromatic Hydrocarbon Emission in the Central Regions of Three Seyferts and the Implication for Underlying Feedback Mechanisms
DOI: 10.3847/2041-8213/ad81d0 Bibcode: 2024ApJ...975L...2Z

Bunker, Andrew J.; Imanishi, Masatoshi; Alonso-Herrero, Almudena +29 more

We analyze JWST Mid-Infrared Instrument/Medium Resolution Spectrograph integral field unit observations of three Seyferts from the Galactic Activity, Torus, and Outflow Survey (GATOS) and showcase the intriguing polycyclic aromatic hydrocarbon (PAH) and emission-line characteristics in regions of ∼500 pc scales over or around their active galactic…

2024 The Astrophysical Journal
JWST 6
Assessing the robustness of the Galactic rotation curve inferred from the Jeans equations using Gaia DR3 and cosmological simulations
DOI: 10.1051/0004-6361/202450911 Bibcode: 2024A&A...692A..50K

Laporte, Chervin F. P.; Helmi, Amina; Antoja, Teresa +2 more

Context. Several authors have recently applied Jeans modelling to Gaia-based datasets to infer the circular velocity curve for the Milky Way. These works have consistently found evidence for a continuous decline in the rotation curve beyond ~15 kpc, which may indicate the existence of a light dark matter (DM) halo. Aims. Using a large sample of Ga…

2024 Astronomy and Astrophysics
Gaia 6