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Extreme Red-wing Enhancements of UV Lines during the 2022 March 30 X1.3 Solar Flare
DOI: 10.3847/1538-4357/acf8c6 Bibcode: 2023ApJ...958...67X

Polito, Vanessa; Xu, Yan; Jing, Ju +3 more

Here, we present the study of a compact emission source during an X1.3 flare on 2022 March 30. Within a ~41 s period (17:34:48 UT to 17:35:29 UT), Interface Region Imaging Spectrograph observations show spectral lines of Mg II, C II, and Si IV with extremely broadened, asymmetric red wings. This source of interest (SOI) is compact, ~1.″6, and is l…

2023 The Astrophysical Journal
IRIS 3
Dark dust. III. The high-quality single-cloud reddening curve sample: Scrutinizing extinction curves in the Milky Way
DOI: 10.1051/0004-6361/202244594 Bibcode: 2023A&A...676A.132S

Krełowski, J.; Siebenmorgen, R.; Chini, Rolf +2 more

The nature of dust in the diffuse interstellar medium can be best investigated by means of reddening curves where only a single interstellar cloud lies between the observer and the background source. Published reddening curves often suffer from various systematic uncertainties. We merged a sample of 820 reddening curves of stars for which both FOR…

2023 Astronomy and Astrophysics
Gaia IUE 3
Applied Machine-Learning Models to Identify Spectral Sub-Types of M Dwarfs from Photometric Surveys
DOI: 10.1088/1538-3873/acc974 Bibcode: 2023PASP..135d4502S

Sithajan, Sirinrat; Meethong, Sukanya

M dwarfs are the most abundant stars in the Solar Neighborhood and they are prime targets for searching for rocky planets in habitable zones. Consequently, a detailed characterization of these stars is in demand. The spectral sub-type is one of the parameters that is used for the characterization and it is traditionally derived from the observed s…

2023 Publications of the Astronomical Society of the Pacific
Gaia 3
A 9 Month Hubble Space Telescope Near-UV Survey of M87. I. Light and Color Curves of 94 Novae, and a Redetermination of the Nova Rate
DOI: 10.3847/1538-4365/ad02fd Bibcode: 2023ApJS..269...42S

Graur, Or; Shara, Michael M.; Meyer, Eileen T. +10 more

M87 has been monitored with a cadence of 5 days over a span of 9 months through the near-ultraviolet (NUV; F275W) and optical (F606W) filters of the Wide Field Camera 3 (WFC3) of the Hubble Space Telescope. This unprecedented dataset yields the NUV and optical light and color curves of 94 M87 novae, characterizing the outburst and decline properti…

2023 The Astrophysical Journal Supplement Series
eHST 3
Global surficial water content stored in hydrated silicates at Mars from OMEGA/MEx
DOI: 10.1016/j.icarus.2023.115537 Bibcode: 2023Icar..39815537R

Poulet, François; Cardesín-Moinelo, Alejandro; Martin, Patrick +2 more

Assessing the water content at the surface of Mars is key to understand the history of water and past climate of the planet but it also is very important for future exploration and potential In Situ Resource Utilization (ISRU). Numerous locations on the surface, known to harbor hydrated minerals, have been detected and their mineralogical assembla…

2023 Icarus
MEx 3
Piercing the dusty veil of hyper-luminous infrared galaxies: Sub-arcsecond 144 MHz ILT observations of HLIRGs in the Lockman Hole
DOI: 10.1051/0004-6361/202244378 Bibcode: 2023A&A...671A..85S

Bondi, M.; Prandoni, I.; Małek, K. +10 more

Context. Hyper-luminous infrared galaxies (HLIRGs) are among the most extreme systems in the Universe. With infrared (IR) luminosities of LIR > 1013 L they can have IR-derived star formation rates (SFRs) exceeding 103 M yr−1. Theoretical models have a hard time reproducing the …

2023 Astronomy and Astrophysics
Herschel 3
On the Periodicities in Solar Rotation and Activity Determined from Sunspot-Group Data and Possible Connection with Rossby-Like Waves
DOI: 10.1007/s11207-023-02114-9 Bibcode: 2023SoPh..298...39R

Hanslmeier, Arnold; Ruždjak, Domagoj; Brajša, Roman +2 more

Analyses of solar rotation and activity, and their variations, can improve the understanding of the formation and interaction of the solar-activity bands and therefore give important observational constraints on the modelling of the solar dynamo and improve the forecast capability in solar activity and space weather. Sunspot-position data obtained…

2023 Solar Physics
SOHO 3
Atmospheric Retrieval of L Dwarfs: Benchmarking Results and Characterizing the Young Planetary Mass Companion HD 106906 b in the Near-infrared
DOI: 10.3847/1538-3881/acfb87 Bibcode: 2023AJ....166..192A

Marley, Mark; Meyer, Michael R.; Quanz, Sascha P. +7 more

We present model constraints on the atmospheric structure of HD 106906 b, a planetary-mass companion orbiting at a ~700 au projected separation around a 15 Myr old stellar binary, using the APOLLO retrieval code on spectral data spanning 1.1-2.5 µm. C/O ratios can provide evidence for companion formation pathways, as such pathways are ambigu…

2023 The Astronomical Journal
eHST 3
Kinetic Features of Alpha Particles in a Pestchek-like Magnetic Reconnection Event in the Solar Wind Observed by Solar Orbiter
DOI: 10.3847/2041-8213/acd553 Bibcode: 2023ApJ...952L..11D

Verscharen, Daniel; He, Jiansen; Fedorov, Andrey +10 more

The acceleration and heating of solar wind particles by magnetic reconnection are important mechanisms in space physics. Although alpha particles (4He2+) are the second most abundant population of solar wind ions, their kinetic behavior in solar wind magnetic reconnection is not well understood. Using the high-energy (1500-30…

2023 The Astrophysical Journal
SolarOrbiter 3
Discovery of five Green pea galaxies with double-peaked narrow [O III] lines
DOI: 10.1093/mnras/stad1857 Bibcode: 2023MNRAS.524.2224L

Zheng, Zhen-Ya; Wang, Jun-Xian; Malhotra, Sangeeta +9 more

Although double-peaked narrow emission-line galaxies have been studied extensively in the past years, only a few are reported with the Green pea (GP) galaxies. Here we present our discovery of five GP galaxies with double-peaked narrow [O III] emission lines, referred to as DPGPs, selected from the LAMOST and SDSS spectroscopic surveys. We find th…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 3