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Galaxies decomposition with spiral arms - II. A multiwavelength case study of M 51
DOI: 10.1093/mnras/stae108 Bibcode: 2024MNRAS.528.1276M

Gontcharov, George A.; Mosenkov, Aleksandr V.; Savchenko, Sergey S. +7 more

Spiral structure can contribute significantly to a galaxy's luminosity. However, only rarely are proper photometric models of spiral arms used in decompositions. As we show in the previous work, including the spirals as a separate component in a photometric model of a galaxy would both allow to obtain their structural parameters, and reduce the sy…

2024 Monthly Notices of the Royal Astronomical Society
Herschel 7
A catalogue of Galactic GEMS: Globular cluster Extra-tidal Mock Stars
DOI: 10.1093/mnras/stae203 Bibcode: 2024MNRAS.528.5189G

Speagle, Joshua S.; Lane, James M. M.; Webb, Jeremy J. +2 more

This work presents the Globular cluster Extra-tidal Mock Star (GEMS) catalogue of extra-tidal stars and binaries created via three-body dynamical encounters in globular cluster cores. Using the particle-spray code Corespray, we sample $N=50\, 000$ extra-tidal stars and escaped recoil binaries for 159 Galactic globular clusters. Sky positions, kine…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 7
Discovery and follow-up of ASASSN-23bd (AT 2023clx): the lowest redshift and luminosity optically selected tidal disruption event
DOI: 10.1093/mnras/stae1121 Bibcode: 2024MNRAS.530.4501H

Kochanek, C. S.; Galbany, L.; Brown, P. J. +23 more

We report the All-Sky Automated Survey for SuperNovae discovery of the tidal disruption event (TDE) ASASSN-23bd (AT 2023clx) in NGC 3799, a LINER galaxy with no evidence of strong active galactic nucleus (AGN) activity over the past decade. With a redshift of z = 0.01107 and a peak ultraviolet (UV)/optical luminosity of (5.4 ± 0.4) × 1042

2024 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST 7
DIAmante TESS AutoRegressive Planet Search (DTARPS). I. Analysis of 0.9 Million Light Curves
DOI: 10.3847/1538-3881/ad29f0 Bibcode: 2024AJ....167..202M

Feigelson, Eric D.; Montalto, Marco; Melton, Elizabeth J. +3 more

Nearly one million light curves from the TESS Year 1 southern hemisphere extracted from Full Field Images with the DIAmante pipeline are processed through the AutoRegressive Planet Search statistical procedure. ARIMA models remove lingering autocorrelated noise, the Transit Comb Filter identifies the strongest periodic signal in the light curve, a…

2024 The Astronomical Journal
Gaia 7
Effects of density and temperature variations on the metallicity of Mrk 71
DOI: 10.1038/s41550-024-02198-8 Bibcode: 2024NatAs...8..275M

Kreckel, Kathryn; Esteban, César; García-Rojas, Jorge +2 more

In a very recent work, [1] claim that the scenario of temperature inhomogeneities proposed by [2] ($t2$ > 0) is not able to explain the O$^{2+}$/H$^{+}$ abundance discrepancy observed between the calculations based on the optical [OIII] collisional excited lines (CELs) and the OII recombination lines (RLs) in the star forming galaxy Mrk71. In t…

2024 Nature Astronomy
Herschel 7
First study of the supernova remnant population in the Large Magellanic Cloud with eROSITA
DOI: 10.1051/0004-6361/202348868 Bibcode: 2024A&A...692A.237Z

Maitra, Chandreyee; Koribalski, Bärbel S.; Sasaki, Manami +11 more

Aims. The all-sky survey carried out by the extended Roentgen Survey with an Imaging Telescope Array (eROSITA) on board Spektrum-Roentgen-Gamma (Spektr-RG, SRG) has provided spatially and spectrally resolved X-ray data of the entire Large Magellanic Cloud (LMC) and its immediate surroundings in the soft X-ray band down to 0.2 keV, with an average …

2024 Astronomy and Astrophysics
XMM-Newton 7
Host-star Properties of Hot, Warm, and Cold Jupiters in the Solar Neighborhood from Gaia Data Release 3: Clues to Formation Pathways
DOI: 10.3847/1538-3881/ad429f Bibcode: 2024AJ....168....7B

Henning, Thomas; Manoj, P.; Narang, Mayank +5 more

Giant planets exhibit diverse orbital properties, hinting at their distinct formation and dynamic histories. In this paper, using Gaia Data Release 3 (DR3), we investigate if and how the orbital properties of Jupiters are linked to their host star properties, particularly their metallicity and age. We obtain metallicities for main-sequence stars o…

2024 The Astronomical Journal
Gaia 7
NOEMA reveals the true nature of luminous red JWST z > 10 galaxy candidates
DOI: 10.1051/0004-6361/202348306 Bibcode: 2024A&A...681L...3M

Walter, F.; Oesch, P. A.; Barrufet, L. +3 more

The first year of JWST has revealed a surprisingly large number of luminous galaxy candidates beyond z > 10. While some galaxies have already been spectroscopically confirmed, there is mounting evidence that a subsample of the candidates with particularly red inferred UV colours are, in fact, lower redshift contaminants. These interlopers are o…

2024 Astronomy and Astrophysics
eHST JWST 7
Not-so-fast Kepler-1513: a perturbing planetary interloper in the exomoon corridor
DOI: 10.1093/mnras/stad3070 Bibcode: 2024MNRAS.527..620Y

Dalba, Paul A.; McLeod, Kim K.; Nesvorný, David +9 more

Transit timing variations (TTVs) can be induced by a range of physical phenomena, including planet-planet interactions, planet-moon interactions, and stellar activity. Recent work has shown that roughly half of moons would induce fast TTVs with a short period in the range of 2-4 orbits of its host planet around the star. An investigation of the Ke…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 7
Characterizing the Rapid Hydrogen Disappearance in SN 2022crv: Evidence of a Continuum between Type Ib and IIb Supernova Properties
DOI: 10.3847/1538-4357/ad710e Bibcode: 2024ApJ...974..316D

Van Dyk, Schuyler D.; Filippenko, Alexei V.; Modjaz, Maryam +52 more

We present optical and near-infrared (NIR) observations of SN 2022crv, a stripped-envelope supernova in NGC 3054, discovered within 12 hr of explosion by the Distance Less Than 40 Mpc Survey. We suggest that SN 2022crv is a transitional object on the continuum between Type Ib supernovae (SNe Ib) and Type IIb supernovae (SNe IIb). A high-velocity h…

2024 The Astrophysical Journal
eHST 7