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A Novel Survey for Young Substellar Objects with the W-band Filter. V. IC 348 and Barnard 5 in the Perseus Cloud
DOI: 10.3847/1538-3881/ac8547 Bibcode: 2022AJ....164..125L

Jose, Jessy; Allers, Katelyn; Albert, Loïc +10 more

We report the discovery of substellar objects in the young star cluster IC 348 and the neighboring Barnard 5 dark cloud, both at the eastern end of the Perseus star-forming complex. The substellar candidates are selected using narrowband imaging, i.e., on and off photometric technique with a filter centered around the water absorption feature at 1…

2022 The Astronomical Journal
Gaia 7
AstroSat/UVIT Cluster Photometry in the Northern Disk of M31
DOI: 10.3847/1538-3881/ac9058 Bibcode: 2022AJ....164..183L

Leahy, Denis; Buick, Megan; Leahy, Cameron

The Andromeda galaxy (M31) is an object of ongoing study with the Ultraviolet Imaging Telescope (UVIT) on AstroSat. UVIT far-UV (FUV) and near-UV (NUV) photometry is carried out here for a set of 239 clusters in the NE disk and bulge of M31 that overlap with the HST/PHAT survey. Padova stellar models were applied to derive ages, masses, metallicit…

2022 The Astronomical Journal
eHST 7
Interplay between Young Stars and Molecular Clouds in the Ophiuchus Star-forming Complex
DOI: 10.3847/1538-3881/ac5cc8 Bibcode: 2022AJ....163..233G

Chen, Wen-Ping; Gupta, Aashish

We present spatial and kinematic correlation between the young stellar population and the cloud clumps in the Ophiuchus star-forming region. The stellar sample consists of known young objects at various evolutionary stages, taken from the literature, some of which are diagnosed with Gaia EDR3 parallax and proper-motion measurements. The molecular …

2022 The Astronomical Journal
Gaia 7
X-Ray Emission from the Exoplanet Hosting LTT 1445 Triple Star System
DOI: 10.3847/1538-3881/ac8f25 Bibcode: 2022AJ....164..206B

Brown, Alexander; France, Kevin; Youngblood, Allison +5 more

JWST will be able to observe the atmospheres of rocky planets transiting nearby M dwarfs. The M-dwarf triple star system LTT 1445, at a distance of 6.86 pc, hosts some of the nearest rocky terrestrial planets. These planets most likely orbit the M 3.5V star LTT 1445A. During a 28.6 ks Chandra ACIS-S3 observation we have: (i) spatially resolved and…

2022 The Astronomical Journal
Gaia eHST 7
Discovery of 34 Low-mass Comoving Systems Using NOIRLab Source Catalog DR2
DOI: 10.3847/1538-3881/ac68e7 Bibcode: 2022AJ....164....3K

Kiman, Rocio; Kirkpatrick, J. Davy; Burgasser, Adam J. +12 more

We present the discovery of 34 comoving systems containing an ultracool dwarf found by means of the NOIRLab Source Catalog (NSC) DR2. NSC's angular resolution of ~ 1″ allows for the detection of small separation binaries with significant proper motions. We used the catalog's accurate proper motion measurements to identify the companions by cross-m…

2022 The Astronomical Journal
Gaia 7
Ages and Masses of Star Clusters in M33: a Multiwavelength Study
DOI: 10.3847/1538-3881/ac324e Bibcode: 2022AJ....163...16M

Calzetti, Daniela; Moeller, Caitlin

We combine archival images for the nearby galaxy M33 (Triangulum Galaxy) from the ultraviolet (UV) to the infrared to derive ages, masses, and extinctions for the young star cluster population, and compare our physical parameters with published ones. Our goal is to test the robustness of clusters ages and masses, and possibly improve on existing o…

2022 The Astronomical Journal
eHST 7
HD 83443c: A Highly Eccentric Giant Planet on a 22 yr Orbit
DOI: 10.3847/1538-3881/ac6589 Bibcode: 2022AJ....163..273E

Kane, Stephen R.; Butler, R. P.; Wittenmyer, Robert A. +20 more

We report the discovery of a highly eccentric long-period Jovian planet orbiting the hot-Jupiter host HD 83443. By combining radial velocity data from four instruments (AAT/UCLES, Keck/HIRES, HARPS, Minerva-Australis) spanning more than two decades, we find evidence for a planet with m sin $i={1.35}_{-0.06}^{+0.07}$ M J, moving on an or…

2022 The Astronomical Journal
Gaia Hipparcos 6
Kinematics of the Central Stars Powering Bowshock Nebulae and the Large Multiplicity Fraction of Runaway OB Stars
DOI: 10.3847/1538-3881/ac7f2b Bibcode: 2022AJ....164...86K

Kobulnicky, Henry A.; Chick, William T.

OB stars powering stellar bowshock nebulae (SBNe) have been presumed to have large peculiar velocities. We measured peculiar velocities of SBN central stars to assess their kinematics relative to the general O-star population using Gaia EDR3 data for 267 SBN central stars and a sample of 455 Galactic O stars to derive projected velocities v 2…

2022 The Astronomical Journal
Gaia 6
SOFIA FEEDBACK Survey: PDR Diagnostics of Stellar Feedback in Different Regions of RCW 49
DOI: 10.3847/1538-3881/ac8a44 Bibcode: 2022AJ....164..150T

Schneider, N.; Stutzki, J.; Tielens, A. G. G. M. +13 more

We quantified the effects of stellar feedback in RCW 49 by determining the physical conditions in different regions using the [C II] 158 µm and [O I] 63 µm observations from SOFIA, the 12CO (3-2) observations from APEX, and the H2 line observations from Spitzer telescopes. Large maps of RCW 49 were observed with t…

2022 The Astronomical Journal
Herschel 6
ARMADA. II. Further Detections of Inner Companions to Intermediate-mass Binaries with Microarcsecond Astrometry at CHARA and VLTI
DOI: 10.3847/1538-3881/ac8eae Bibcode: 2022AJ....164..184G

Gies, Douglas R.; Monnier, John D.; Lanthermann, Cyprien +18 more

We started a survey with CHARA/MIRC-X and VLTI/GRAVITY to search for low-mass companions orbiting individual components of intermediate-mass binary systems. With the incredible precision of these instruments, we can detect astrometric "wobbles" from companions down to a few tens of microarcseconds. This allows us to detect any previously unseen tr…

2022 The Astronomical Journal
Gaia 6