Search Publications

Hubble Detects the Start of a New Saturn Ring Spoke Season
DOI: 10.1029/2022GL101904 Bibcode: 2023GeoRL..5001904S

Nicholson, Philip D.; Hedman, Matthew M.; Showalter, Mark R. +4 more

Saturn's ring spokes typically appear over an 8-year duration centered on equinox. Hubble Space Telescope observations in 2021 indicate the beginning of a new spoke season as Saturn approaches equinox in 2025. The spokes show increased contrast and longevity in 2022, persisting for up to 11 hours. The spokes are visible from UV to near-IR and are …

2023 Geophysical Research Letters
eHST 2
Modeling the Chromosphere and Transition Region of Planet-hosting Star GJ 436
DOI: 10.3847/1538-4357/ace103 Bibcode: 2023ApJ...954...73H

Peacock, Sarah; Barman, Travis; Hatzes, Artie P. +12 more

Ahead of upcoming space missions intending to conduct observations of low-mass stars in the ultraviolet (UV) spectral region it becomes imperative to simultaneously conduct atmospheric modeling from the UV to the visible (VIS) and near-infrared (NIR). Investigations on extended spectral regions will help to improve the overall understanding of the…

2023 The Astrophysical Journal
eHST 2
Searching for signatures of H α spicule-like features in the solar transition region
DOI: 10.1093/mnras/stad1742 Bibcode: 2023MNRAS.524.1156V

Shetye, Juie; Doyle, J. Gerry; Vilangot Nhalil, Nived

New instruments and telescopes covering the optical and ultraviolet spectral regions have revealed a range of small-scale dynamic features, many which may be related. For example, the range of spicule-like features hints towards a spectrum of features and not just two types; however, direct observational evidence in terms of tracking spicules acro…

2023 Monthly Notices of the Royal Astronomical Society
IRIS 2
Spectroscopic study of Herbig Ae/Be stars in the Galactic anti-centre region from LAMOST DR5
DOI: 10.1093/mnras/stad2067 Bibcode: 2023MNRAS.524.5166N

Arun, R.; Mathew, Blesson; Kartha, Sreeja S. +3 more

We study a sample of 119 Herbig Ae/Be stars in the Galactic anti-centre direction using the spectroscopic data from large sky area multi-object fiber spectroscopic telescope survey program. Emission lines of hydrogen belonging to the Balmer and Paschen series, and metallic lines of species such as Fe II, O I, Ca II triplet are identified. A modera…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 2
Testing the planetary hypothesis of NY Virginis: anticipated change in the eclipse timing trend within the next five years
DOI: 10.1093/mnras/stad2648 Bibcode: 2023MNRAS.525.6050E

Baştürk, Özgür; Esmer, Ekrem Murat; Selam, Selim Osman

Regarding the recent debate about the potential circumbinary exoplanets around NY Virginis (NY Vir), we analysed mid-eclipse timings of NY Vir using archival photometric data as well as our own observations and the ones from TESS. For this purpose, we first modelled the available eclipse light curves of the binary system to determine the masses of…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 2
LBT-MODS spectroscopy of high-redshift candidates in the Chandra J1030 field. A newly discovered z ∼ 2.8 large-scale structure
DOI: 10.1051/0004-6361/202245513 Bibcode: 2023A&A...673A..97M

Comastri, Andrea; Signorini, Matilde; Vito, Fabio +13 more

We present the results of a spectroscopic campaign with the Multi-Object Double Spectrograph (MODS) instrument mounted on the Large Binocular Telescope (LBT), aimed at obtaining a spectroscopic redshift for seven Chandra J1030 sources with a photometric redshift ≥2.7 and optical magnitude rAB = [24.5 − 26.5]. We obtained a spectroscopic…

2023 Astronomy and Astrophysics
eHST 2
Massive Hypervelocity Runaway Stars in the Large Magellanic Cloud
DOI: 10.3847/1538-4357/acd644 Bibcode: 2023ApJ...952...64L

Xu, Ye; Liu, Dejian; Hao, Chaojie +3 more

Since the hypervelocity stars were discovered in the Milky Way, various mechanisms have been proposed to explain these runaway stars. Up to now, however, the dominant ejected mechanism of hypervelocity stars is still unclear. As the largest and closest face-on satellite galaxy of the Milky Way, the Large Magellanic Cloud (LMC) serves as a good tar…

2023 The Astrophysical Journal
Gaia 2
NuSTAR Hard X-Ray Monitoring of Gravitationally Lensed Quasar RX J1131-1231
DOI: 10.3847/1538-4357/ad0ced Bibcode: 2023ApJ...959..101D

Zoghbi, Abderahmen; Dai, Xinyu; Morgan, Christopher W. +2 more

The X-ray emission from active galactic nuclei is believed to come from a combination of inverse Compton scattering of photons from the accretion disk and reprocessing of the direct X-ray emission by reflection. We present hard (10-80 keV) and soft (0.5-8 keV) X-ray monitoring of a gravitationally lensed quasar RX J1131-1231 (hereafter RXJ1131) wi…

2023 The Astrophysical Journal
XMM-Newton 2
CHEX-MATE: X-ray absorption and molecular content of the interstellar medium toward galaxy clusters
DOI: 10.1051/0004-6361/202347143 Bibcode: 2023A&A...678A.181B

Pointecouteau, E.; Pratt, G. W.; Rossetti, M. +14 more

The X-ray spectrum of extragalactic sources, such as galaxy clusters, is affected by the photo-absorption of various components of the Galactic interstellar medium (ISM). The resulting spectral distortion contributes to the systematics of cluster temperature measurements. It essentially depends on the neutral (atomic+molecular) Galactic hydrogen d…

2023 Astronomy and Astrophysics
XMM-Newton 2
A clustering study of the old open cluster Trumpler 19
DOI: 10.1007/s10509-023-04228-9 Bibcode: 2023Ap&SS.368...73G

Gao, Xinhua; Fang, Dan

In this paper, we investigate the spatial structure and dynamical state of the poorly studied old (4 Gyr) open cluster Trumpler 19 based on reliable cluster members from Ga

2023 Astrophysics and Space Science
Gaia 2