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Firmamento: A Multimessenger Astronomy Tool for Citizen and Professional Scientists
DOI: 10.3847/1538-3881/ad216a Bibcode: 2024AJ....167..116T

Giommi, Paolo; Doro, Michele; Pollock, A. M. T. +12 more

Firmamento (https://firmamento.hosting.nyu.edu) is a new-concept, web-based, and mobile-friendly data analysis tool dedicated to multifrequency/multimessenger emitters, as exemplified by blazars. Although initially intended to support a citizen researcher project at New York University–Abu Dhabi, Firmamento has evolved to be a valuable tool for pr…

2024 The Astronomical Journal
XMM-Newton 4
Evolution of the Local Spiral Structure Revealed by OB-type Stars in Gaia DR3
DOI: 10.3847/1538-3881/ad5201 Bibcode: 2024AJ....168...25G

Hao, C. J.; Hou, L. G.; Lin, Z. H. +5 more

The structure and evolution of the spiral arms of the Milky Way have long been an important yet controversial issue. The wide age range of OB-type stars, coupled with the large amount of high-precision astrometric data provided by Gaia DR3, presents us with an opportunity to explore this issue. After constructing overdensity maps and examining the…

2024 The Astronomical Journal
Gaia 4
UVIT Study of the MAgellanic Clouds (U-SMAC). II. A Far-UV Catalog of the Small Magellanic Cloud: Morphology and Kinematics of Young Stellar Population
DOI: 10.3847/1538-3881/ad7de2 Bibcode: 2024AJ....168..255H

Subramaniam, Annapurni; Subramanian, Smitha; Nayak, Prasanta K. +1 more

The Small Magellanic Cloud (SMC) is an irregular dwarf galaxy that has recently undergone an interaction with the Large Magellanic Cloud. The young massive stars in the SMC formed in the disturbed low-metallicity environment are important targets in astrophysics. We present a catalog of ∼76,800 far-ultraviolet (FUV) sources toward the SMC detected…

2024 The Astronomical Journal
Gaia 4
Circumstellar Disk Accretion Across the Lagoon Nebula: The Influence of Environment and Stellar Mass
DOI: 10.3847/1538-3881/ad1f65 Bibcode: 2024AJ....167..120V

Howell, Steve B.; Cody, Ann Marie; Beccari, Giacomo +9 more

Pre-main-sequence disk accretion is pivotal for determining the final stellar properties and the early conditions for close-in planets. We aim to establish the impact of internal (stellar mass) and external (radiation field) parameters on the disk evolution in the Lagoon Nebula massive star-forming region. We employ simultaneous u, g, r, i, Hα tim…

2024 The Astronomical Journal
Gaia 4
A Census of the β Pic Moving Group and Other Nearby Associations with Gaia
DOI: 10.3847/1538-3881/ad697d Bibcode: 2024AJ....168..159L

Luhman, K. L.

I have used the third data release of the Gaia mission to improve the reliability and completeness of membership samples in the β Pic moving group (BPMG) and other nearby associations with ages of 20–50 Myr (Sco Body, Carina, Columba, χ 1 For, Tuc-Hor, IC 2602, IC 2391, NGC 2547). I find that Carina, Columba, and χ 1 For are …

2024 The Astronomical Journal
Gaia 4
Shadowing in the Protoplanetary Disk of ZZ Tau IRS with HST
DOI: 10.3847/1538-3881/ad1b5e Bibcode: 2024AJ....167...75H

Dong, Ruobing; Liu, Hauyu Baobab; Hashimoto, Jun +2 more

An inner component misaligned from an outer component in a protoplanetary disk can result in the former casting shadows on the latter. We present a new instance of shadowing on the outer disk around a very-low-mass star, ZZ Tau IRS. Through the analysis of near-infrared (NIR) archival data at λ = 1.6 µm acquired with the Wide Field Camera 3 …

2024 The Astronomical Journal
Gaia eHST 4
JWST/NIRCam Imaging of Young Stellar Objects. I. Constraints on Planets Exterior to the Spiral Disk Around MWC 758
DOI: 10.3847/1538-3881/ad11d5 Bibcode: 2024AJ....167..181W

Dong, Ruobing; Wolff, Schuyler G.; Johnstone, Doug +18 more

MWC 758 is a young star hosting a spiral protoplanetary disk. The spirals are likely companion-driven, and two previously identified candidate companions have been identified—one at the end the Southern spiral arm at ∼0.″6, and one interior to the gap at ∼0.″1. With JWST/NIRCam, we provide new images of the disk and constraints on planets exterior…

2024 The Astronomical Journal
JWST 4
Chemical Homogeneity of Wide Binary Systems: An Approach from Near-Infrared Spectroscopy
DOI: 10.3847/1538-3881/ad0a62 Bibcode: 2024AJ....167....3L

Lee, Young-Wook; Koch-Hansen, Andreas J.; Hong, Seungsoo +2 more

Wide binaries, with separations between the two stars from a few au to more than several thousand au, are valuable objects for various research topics in Galactic astronomy. As the number of newly reported wide binaries continues to increase, studying the chemical abundances of their component stars becomes more important. We conducted high-resolu…

2024 The Astronomical Journal
Gaia 4
HATS-38 b and WASP-139 b Join a Growing Group of Hot Neptunes on Polar Orbits
DOI: 10.3847/1538-3881/ad70b8 Bibcode: 2024AJ....168..185E

Jordán, Andrés; Brahm, Rafael; Boyle, Gavin +9 more

We constrain the sky-projected obliquities of two low-density hot Neptune planets, HATS-38 b and WASP-139 b, orbiting nearby G and K stars using Rossiter–McLaughlin (RM) observations with VLT/ESPRESSO, yielding λ=108

2024 The Astronomical Journal
Gaia 4
A Data-driven Search For Mid-infrared Excesses Among Five Million Main-sequence FGK Stars
DOI: 10.3847/1538-3881/ad6b90 Bibcode: 2024AJ....168..157C

Hogg, David W.; Contardo, Gabriella

Stellar infrared excesses can indicate various phenomena of interest, from protoplanetary disks to debris disks, or (more speculatively) techno-signatures along the lines of Dyson spheres. In this paper, we conduct a large search for "extreme" infrared excesses, designed as a data-driven contextual anomaly detection pipeline. We focus our search o…

2024 The Astronomical Journal
Gaia 4