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Electron Density Distribution in H II Regions in IC 10
DOI: 10.3847/1538-3881/ad597a Bibcode: 2024AJ....168..117P

Lebouteiller, Vianney; Ramambason, Lise; Jackson, James M. +7 more

We present the [O III] λ52 µm map of the dwarf galaxy IC 10 obtained with the Field-Imaging Far-Infrared Line Spectrometer on board the Stratospheric Observatory for Infrared Astronomy. We combine the [O III] λ52 µm map with Herschel and Spitzer observations to estimate the electron density distribution of the brightest H II regions of…

2024 The Astronomical Journal
Herschel 1
A Phenomenon Resembling Early Superhumps in a New SU UMa-type Dwarf Nova with a 2 hr Orbital Period
DOI: 10.3847/1538-3881/acf718 Bibcode: 2024AJ....167...71B

Garnavich, Peter; Littlefield, Colin; Szkody, Paula +4 more

We investigate K2BS5, an optical transient that we identified in Campaign 13 of the Kepler/K2 archives by the K2 Background Survey, and classify it as a new SU UMa-type dwarf nova. Using the light curve generated from Keplers long-cadence observation mode, we analyze the dwarf nova during quiescence and superoutburst. Following 20 days of quiescen…

2024 The Astronomical Journal
Gaia XMM-Newton 1
Frequencies of Warm Debris Disks Based on Point Source Catalogs of Spitzer, WISE, and Gaia
DOI: 10.3847/1538-3881/ad3df8 Bibcode: 2024AJ....167..275M

Momose, Munetake; Mizuki, Toshiyuki; Aizawa, Masataka +1 more

More than a thousand warm debris disks have been detected as infrared excess at mid-infrared wavelengths, and their frequencies have been obtained for various spectral types of stars. However, the dependence of the frequencies on spectral type is still debated because the number of stars with significant and detectable infrared excess is limited. …

2024 The Astronomical Journal
AKARI Gaia 1
Planet Hunters NGTS: New Planet Candidates from a Citizen Science Search of the Next Generation Transit Survey Public Data
DOI: 10.3847/1538-3881/ad32c8 Bibcode: 2024AJ....167..238O

Wheatley, Peter J.; Bayliss, Daniel; Schwamb, Megan E. +36 more

We present the results from the first two years of the Planet Hunters Next Generation Transit Survey (NGTS) citizen science project, which searches for transiting planet candidates in data from the NGTS by enlisting the help of members of the general public. Over 8000 registered volunteers reviewed 138,198 light curves from the NGTS Public Data Re…

2024 The Astronomical Journal
Gaia 1
Orbits of Binary Stars: from Visual Measures to Speckle Interferometry
DOI: 10.3847/1538-3881/ad72e5 Bibcode: 2024AJ....168..190T

Tokovinin, Andrei

Knowledge of the orbits of visual binary stars has always been one of the fundamentals of astronomy. Based historically on the visual measures, nowadays the orbits rely more (or exclusively) on the accurate speckle data. This prompts reconsideration of the methods of orbit calculation, undertaken here and illustrated by 20 examples, from accurate …

2024 The Astronomical Journal
Gaia 1
Is the RSGC4 (Alicante 8) Cluster a Real Star Cluster? Peculiar Radial Velocities of Red Supergiant Stars
DOI: 10.3847/1538-3881/ad35ad Bibcode: 2024AJ....167..230C

Lee, Jae-Joon; Myeong, GyuChul; Oh, Heeyoung +1 more

Young massive star clusters, like the six red supergiant clusters in the Scutum complex, provide valuable insights into star formation and galaxy structures. We investigated the high-resolution near-infrared spectra of 60 RSG candidates in these clusters using the Immersion Grating Infrared Spectrograph. Among the candidates in RSGC4, we found sig…

2024 The Astronomical Journal
Gaia 1
Oxygen Abundance Throughout the Dwarf Starburst Galaxy IC 10
DOI: 10.3847/1538-3881/ad7f3c Bibcode: 2024AJ....168..250C

Sandstrom, Karin; Armus, Lee; Runco, Jordan N. +5 more

Measurements of oxygen abundance throughout galaxies provide insight to the formation histories and ongoing processes. Here we present a study of the gas-phase oxygen abundance in the H II regions and diffuse gas of the nearby starburst dwarf galaxy, IC 10. Using the Keck Cosmic Web Imager at W. M. Keck Observatory, we map the central region of IC…

2024 The Astronomical Journal
eHST 1
The Discovery of Three Galactic Wolf–Rayet Stars
DOI: 10.3847/1538-3881/ad7092 Bibcode: 2024AJ....168..167M

Massey, Philip; Skiff, Brian A.; Marin, Laurella C. +1 more

Wolf–Rayet stars (WRs) are evolved massive stars in the brief stage before they undergo core collapse. Not only are they rare, but they also can be particularly difficult to find due to the high extinction in the Galactic plane. This paper discusses the discovery of three new Galactic WRs previously classified as Hα emission stars, but thanks to G…

2024 The Astronomical Journal
Gaia 1
Searching the SN 1987A SETI Ellipsoid with TESS
DOI: 10.3847/1538-3881/ad2064 Bibcode: 2024AJ....167..101C

Davenport, James R. A.; Siemion, Andrew P. V.; Cody, Ann Marie +4 more

The SETI Ellipsoid is a strategy for technosignature candidate selection that assumes that extraterrestrial civilizations who have observed a galactic-scale event—such as supernova 1987A—may use it as a Schelling point to broadcast synchronized signals indicating their presence. Continuous wide-field surveys of the sky offer a powerful new opportu…

2024 The Astronomical Journal
Gaia 1
Searching for Neutral Hydrogen Escape from the 120 Myr Old Sub-Neptune HIP94235b using HST
DOI: 10.3847/1538-3881/ad6a53 Bibcode: 2024AJ....168..141M

Mayorga, L. C.; Zhou, George; Wittenmyer, Robert A. +9 more

HIP94235 b, a 120 Myr old sub-Neptune, provides us the unique opportunity to study mass loss at a pivotal stage of the system's evolution: the end of a 100 Myr old phase of intense XUV irradiation. We present two observations of HIP94235 b using the Hubble Space Telescope's Space Telescope Imaging Spectrograph in the Lyα wavelength region. We do n…

2024 The Astronomical Journal
eHST 1