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Nine new M dwarf planet candidates from TESS including five gas giants
DOI: 10.1093/mnras/stae1496 Bibcode: 2024MNRAS.531.5053E

Kunimoto, Michelle; Eschen, Yoshi Nike Emilia

We present the detection of nine new planet candidates orbiting M dwarfs, identified using an independent search and vetting pipeline applied to TESS Full-Frame Image data from Sectors 1 to 63. Our candidates include planets as small as 1.4 $\mathrm{ R}_{{\oplus }}$, with orbital periods up to 20 d. Among the nine new candidates, we identified fiv…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 2
Physical properties of trans-Neptunian object (143707) 2003 UY117 derived from stellar occultation and photometric observations
DOI: 10.1051/0004-6361/202451329 Bibcode: 2024A&A...691A..31K

Pallé, E.; Souami, D.; Alvarez-Candal, A. +49 more

Context. Trans-Neptunian objects (TNOs) are considered to be among the most primitive objects in our Solar System. Knowledge of their primary physical properties is essential for understanding their origin and the evolution of the outer Solar System. In this context, stellar occultations are a powerful and sensitive technique for studying these di…

2024 Astronomy and Astrophysics
Gaia 2
Four new eclipsing accreting ultracompact white dwarf binaries found with the Zwicky Transient Facility
DOI: 10.1051/0004-6361/202349010 Bibcode: 2024A&A...683L..10K

Drake, A. J.; Bloom, J. S.; Kulkarni, S. R. +10 more

Context. Accreting ultracompact white dwarf binaries contain a white dwarf that is accreting from a degenerate object. They have orbital periods shorter than 65 min.
Aims: We report the discovery and the orbital period of four new eclipsing accreting ultracompact white dwarf binaries found using the Zwicky Transient Facility (ZTF) and discuss…

2024 Astronomy and Astrophysics
Gaia 2
Non-conventional approach for deriving the radial sizes of coronal mass ejections at different instances: discrepancies in the estimates between remote and in situ observations
DOI: 10.1093/mnras/stae2260 Bibcode: 2024MNRAS.534.2458A

Mishra, Wageesh; Agarwal, Anjali

Understanding the evolution of radial sizes and instantaneous expansion speeds of coronal mass ejections (CMEs) is crucial for assessing their impact duration on Earth's environment. We introduce a non-conventional approach to derive the CME's radial sizes and expansion speeds at different instances during its passage over a single-point in situ s…

2024 Monthly Notices of the Royal Astronomical Society
SOHO 2
A 9 Month Hubble Space Telescope Near-UV Survey of M87. II. A Strongly Enhanced Nova Rate near the Jet of M87
DOI: 10.3847/1538-4357/ad70b7 Bibcode: 2024ApJ...973..144L

Shara, Michael M.; Sparks, William; Lessing, Alec M. +3 more

The 135 classical novae that we have discovered in M87 with two Hubble Space Telescope imaging surveys appear to be strongly concentrated along that galaxy's jet. Detailed simulations show that the likelihood that this distribution occurred by chance is of order 0.3%. The novae near the jet display outburst characteristics (peak luminosities, colo…

2024 The Astrophysical Journal
Gaia eHST 2
Revisiting the local interstellar radiation field using Gaia DR3
DOI: 10.1051/0004-6361/202451086 Bibcode: 2024A&A...691A.330B

Bianchi, S.

Context. Dust grains in the interstellar medium are heated by the integrated radiation from stars in the Milky Way. Thus, knowledge of the local interstellar radiation field (LISRF) is necessary to interpret observations of dust emission in the infrared and constrain (some) properties of interstellar grains. The LISRF representation that is most w…

2024 Astronomy and Astrophysics
Gaia 2
An empirical isochrone archive for nearby open clusters
DOI: 10.1051/0004-6361/202347701 Bibcode: 2024A&A...690A..16R

Meingast, Stefan; Rottensteiner, Alena

Context. The ages of star clusters and co-moving stellar groups contain essential information about the Milky Way. Their special properties and placement throughout the galactic disk make them excellent tracers of galactic structure and key components to unlocking its star formation history. Yet, even though the importance of stellar population ag…

2024 Astronomy and Astrophysics
Gaia 2
Implications on star formation rate indicators from H II regions and diffuse ionized gas in the M101 Group
DOI: 10.1093/mnras/stae1153 Bibcode: 2024MNRAS.530.4560W

Watkins, A. E.; Mihos, J. C.; Harding, P. +1 more

We examine the connection between diffuse ionized gas (DIG), H II regions, and field O and B stars in the nearby spiral M101 and its dwarf companion NGC 5474 using ultra-deep H α narrow-band imaging and archival GALEX UV imaging. We find a strong correlation between DIG H α surface brightness and the incident ionizing flux leaked from the nearby H…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 2
IRIS2+: A Comprehensive Database of Stratified Thermodynamic Models in the Low Solar Atmosphere
DOI: 10.3847/1538-4365/ad1e55 Bibcode: 2024ApJS..271...24S

De Pontieu, Bart; Gošić, Milan; Sainz Dalda, Alberto +1 more

We present the most comprehensive collection of stratified-in-optical-depth thermodynamic models of the lower solar atmosphere. This database, named IRIS2+, consists of 40,320 synthetic representative profiles (RPs) and their corresponding representative model atmospheres (RMAs). The latter result from inverting the observed RPs, which …

2024 The Astrophysical Journal Supplement Series
IRIS 2
Solar Eruptive Phenomena Associated with Solar Energetic Electron Spectral Types
DOI: 10.3847/1538-4357/ad47be Bibcode: 2024ApJ...969..164W

Krucker, Säm; Wimmer-Schweingruber, Robert F.; Wang, Linghua +3 more

The energy spectral shape of solar energetic electron events carries important information on the energetic electron source/acceleration at the Sun. We investigate the association of six newly identified solar energetic electron spectral types with solar eruptive phenomena, including the downward double-power-law (DDPL) spectrum with break energy …

2024 The Astrophysical Journal
SOHO 2