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A Study of Stellar Spins in 15 Open Clusters
DOI: 10.3847/1538-4357/acad7b Bibcode: 2023ApJ...944...39H

Schlaufman, Kevin C.; Healy, Brian F.; McCullough, P. R. +1 more

We analyze spectroscopic and photometric data to determine the projected inclinations of stars in 11 open clusters, placing constraints on the spin-axis distributions of six clusters. We combine these results with four additional clusters studied by Healy & McCullough and Healy et al. to perform an ensemble analysis of their spins. We find tha…

2023 The Astrophysical Journal
Gaia 9
Spectroscopic Confirmation of a Population of Isolated, Intermediate-mass Young Stellar Objects
DOI: 10.3847/1538-3881/ac9314 Bibcode: 2023AJ....165....3K

Zucker, Catherine; Hillenbrand, Lynne A.; Povich, Matthew S. +9 more

Wide-field searches for young stellar objects (YSOs) can place useful constraints on the prevalence of clustered versus distributed star formation. The Spitzer/IRAC Candidate YSO (SPICY) catalog is one of the largest compilations of such objects (~120,000 candidates in the Galactic midplane). Many SPICY candidates are spatially clustered, but, per…

2023 The Astronomical Journal
Gaia 9
WISDOM Project - XV. Giant molecular clouds in the central region of the barred spiral galaxy NGC 5806
DOI: 10.1093/mnras/stad1211 Bibcode: 2023MNRAS.522.4078C

Williams, Thomas G.; Cappellari, Michele; Davis, Timothy A. +7 more

We present high spatial resolution (≈24 pc) Atacama Large Millimeter/sub-millimeter Array 12CO(2-1) observations of the central region of the nearby barred spiral galaxy NGC 5806. NGC 5806 has a highly structured molecular gas distribution with a clear nucleus, a nuclear ring, and offset dust lanes. We identify 170 spatially and spectra…

2023 Monthly Notices of the Royal Astronomical Society
eHST 9
Comprehensive Analysis of the Open Cluster Collinder 74
DOI: 10.48550/arXiv.2310.13582 Bibcode: 2023PARep...1...65Y

Yontan, Talar; Canbay, Remziye

In this study, we have used the Gaia Third Data Release (Gaia DR3) to investigate an intermediate-age open cluster Collinder 74. We have identified 102 probable cluster members by considering stars with a membership probability exceeding 0.5 and located within the designated confinement radius. The mean proper-motion components of Collinder 74 are…

2023 Physics and Astronomy Reports
Gaia 9
Revising Properties of Planet-Host Binary Systems. III. There Is No Observed Radius Gap for Kepler Planets in Binary Star Systems
DOI: 10.3847/1538-3881/acbdf9 Bibcode: 2023AJ....165..177S

Huber, Daniel; Berger, Travis A.; Gaidos, Eric +7 more

Binary stars are ubiquitous; the majority of solar-type stars exist in binaries. Exoplanet occurrence rate is suppressed in binaries, but some multiples do still host planets. Binaries cause observational biases in planet parameters, with undetected multiplicity causing transiting planets to appear smaller than they truly are. We have analyzed the…

2023 The Astronomical Journal
Gaia 9
Small-scale loops heated to transition region temperatures and their chromospheric signatures in the simulated solar atmosphere
DOI: 10.1051/0004-6361/202245390 Bibcode: 2023A&A...672A..47S

Leenaarts, J.; Danilovic, S.; Rempel, M. +2 more

Context. Recent observations have revealed loop-like structures at very small scales visible in observables that sample the transition region (TR) and even coronal temperatures. These structures are referred to as either `unresolved fine structures', `dynamic cool loops', `miniature hot loops' or `campfires' depending on the observables in which t…

2023 Astronomy and Astrophysics
IRIS 9
TOI-1416: A system with a super-Earth planet with a 1.07 d period
DOI: 10.1051/0004-6361/202346370 Bibcode: 2023A&A...677A..12D

Fridlund, M.; Pallé, E.; Guenther, E. W. +49 more

TOI-1416 (BD+42 2504, HIP 70705) is a V =10 late G- or early K-type dwarf star. TESS detected transits in its Sectors 16, 23, and 50 with a depth of about 455 ppm and a period of 1.07 days. Radial velocities (RVs) confirm the presence of the transiting planet TOI-1416 b, which has a mass of 3.48 ± 0.47 M and a radius of 1.62 ± 0.08 R

2023 Astronomy and Astrophysics
Gaia 9
The young mini-Neptune HD 207496b that is either a naked core or on the verge of becoming one
DOI: 10.1051/0004-6361/202245741 Bibcode: 2023A&A...673A...4B

Deleuil, M.; Winn, J. N.; Adibekyan, V. +39 more


Aims: We report the discovery and characterisation of the transiting mini-Neptune HD 207496 b (TOI-1099) as part of a large programme that aims to characterise naked core planets.
Methods: We obtained HARPS spectroscopic observations, one ground-based transit, and high-resolution imaging which we combined with the TESS photometry to conf…

2023 Astronomy and Astrophysics
Gaia XMM-Newton 9
On the Physical Nature of the so-Called Prominence Tornadoes
DOI: 10.1007/s11214-023-00976-w Bibcode: 2023SSRv..219...33G

Heinzel, Petr; Schmieder, Brigitte; Labrosse, Nicolas +7 more

The term `tornado' has been used in recent years to describe several solar phenomena, from large-scale eruptive prominences to small-scale photospheric vortices. It has also been applied to the generally stable quiescent prominences, sparking a renewed interest in what historically was called `prominence tornadoes'. This paper carries out an in-de…

2023 Space Science Reviews
Hinode 9
The Evaporating Massive Embedded Stellar Cluster IRS 13 Close to Sgr A*. I. Detection of a Rich Population of Dusty Objects in the IRS 13 Cluster
DOI: 10.3847/1538-4357/acf6b5 Bibcode: 2023ApJ...956...70P

Eckart, Andreas; Zajaček, Michal; Labadie, Lucas +6 more

A detailed analysis of the nuclear star cluster not only concedes the existence of the S cluster, with its fast-moving stars and the supermassive black hole Sgr A*. It also reveals an embedded region of gas and dust with an exceptionally high stellar density called IRS 13. The IRS 13 cluster can be divided into the northern and eastern counterpart…

2023 The Astrophysical Journal
JWST 9