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Different higher order kinematics between star-forming and quiescent galaxies based on the SAMI, MAGPI, and LEGA-C surveys
DOI: 10.1093/mnras/stac3536 Bibcode: 2023MNRAS.525.2765D

Bell, Eric F.; Übler, Hannah; D'Eugenio, Francesco +38 more

We present the first statistical study of spatially integrated non-Gaussian stellar kinematics spanning 7 Gyr in cosmic time. We use deep, rest-frame optical spectroscopy of massive galaxies (stellar mass $M_\star \gt 10^{10.5} \, \mathrm{M_\odot }$) at redshifts z = 0.05, 0.3, and 0.8 from the SAMI, MAGPI, and LEGA-C surveys, to measure the exces…

2023 Monthly Notices of the Royal Astronomical Society
eHST 7
M92 (NGC 6341) Is a Metal-complex Globular Cluster with an Atypical Primordial Population
DOI: 10.3847/2041-8213/acd05a Bibcode: 2023ApJ...948L..16L

Lee, Jae-Woo

We present a multiple stellar population study of the metal-poor globular cluster (GC) M92 (NGC 6341), which is long known for the substantial metallicity dispersion, using our own photometric system. We find two groups with slightly different mean metallicities, the metal-poor (MP) stars with [Fe/H] hk = -2.412 ± 0.03 and the metal-ri…

2023 The Astrophysical Journal
Gaia eHST 7
Mapping the Decline with Redshift of Dusty Star-forming Galaxies Using JWST and SCUBA-2
DOI: 10.3847/1538-4357/acedae Bibcode: 2023ApJ...956...95B

Barger, A. J.; Cowie, L. L.

We use JWST NIRCam observations of the massive lensing cluster field A2744 to develop a red galaxy selection of f F444W > 1 µJy and f F444W/f F150W > 3.5 that picks out all nine >4.5σ Atacama Large Millimeter/submillimeter Array 1.1 or 1.2 mm sources and 17 of the 19 >5σ SCUBA-2 850 µm sourc…

2023 The Astrophysical Journal
JWST 7
Star formation efficiency and AGN feedback in narrow-line Seyfert 1 galaxies with fast X-ray nuclear winds
DOI: 10.1093/mnras/stad2116 Bibcode: 2023MNRAS.524.3130S

Feruglio, C.; García-Burillo, S.; Krongold, Y. +7 more

We present the first systematic study of the molecular gas and star formation efficiency in a sample of ten narrow-line Seyfert 1 galaxies selected to have X-ray Ultra Fast Outflows and, therefore, to potentially show AGN feedback effects. CO observations were obtained with the IRAM 30-m telescope in six galaxies and from the literature for four g…

2023 Monthly Notices of the Royal Astronomical Society
Herschel eHST 7
Much ado about no offset - characterizing the anomalous multiple-image configuration and the model-driven displacement between light and mass in the multiplane strong lens Abell 3827
DOI: 10.1093/mnras/stad2800 Bibcode: 2023MNRAS.526.2776L

Griffiths, Richard E.; Wagner, Jenny; Lin, Joyce

Abell 3827 is a unique galaxy cluster with a dry merger in its core causing a highly resolved multiple-image configuration of a blue spiral galaxy at zs = 1.24. The surface brightness profiles of four merging galaxies around zd = 0.099 complicate a clear identification of the number of images and finding corresponding small-s…

2023 Monthly Notices of the Royal Astronomical Society
eHST 7
Resolving the binary components of the outbursting protostar HBC 494 with ALMA
DOI: 10.1093/mnras/stad1614 Bibcode: 2023MNRAS.523.4970N

Herczeg, Gregory J.; Zhu, Zhaohuan; Pérez, Sebastián +15 more

Episodic accretion is a low-mass pre-main sequence phenomenon characterized by sudden outbursts of enhanced accretion. These objects are classified into two: protostars with elevated levels of accretion that lasts for decades or more, called FUors, and protostars with shorter and repetitive bursts, called EXors. HBC 494 is a FUor object embedded i…

2023 Monthly Notices of the Royal Astronomical Society
Herschel 7
A multi-technique approach to identifying and/or constraining radial-velocity substellar companions
DOI: 10.1051/0004-6361/202346612 Bibcode: 2023A&A...678A.107P

Kiefer, F.; Lagrange, A. -M.; Rubini, P. +3 more

Context. Although more than one thousand substellar companions have already been detected with the radial velocity (RV) method, many new companions remain to be detected in the public RV archives.
Aims: We wish to use the archival data obtained with the ESO/HARPS spectrograph to search for substellar companions.
Methods: We used the astr…

2023 Astronomy and Astrophysics
Gaia Hipparcos 7
X-shooter survey of young intermediate-mass stars - I. Stellar characterization and disc evolution
DOI: 10.1093/mnras/stac3619 Bibcode: 2023MNRAS.519.3958I

Pascucci, Ilaria; Petr-Gotzens, Monika G.; Panić, Olja +6 more

Intermediate-mass stars (IMSs) represent the link between low-mass and high-mass stars, and cover a key mass range for giant planet formation. In this paper, we present a spectroscopic survey of 241 young IMS candidates with IR-excess, the most complete unbiased sample to date within 300 pc. We combined VLT/X-Shooter spectra with BVR photometric o…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 7
A Statistical Study of IRIS Observational Signatures of Nanoflares and Nonthermal Particles
DOI: 10.3847/1538-4357/acb7da Bibcode: 2023ApJ...945..143C

Polito, Vanessa; Testa, Paola; De Pontieu, Bart +1 more

Nanoflares are regarded as one of the major mechanisms of magnetic energy release and coronal heating in the solar outer atmosphere. We conduct a statistical study on the response of the chromosphere and transition region to nanoflares, as observed by the Interface Region Imaging Spectrograph (IRIS), by using an algorithm for the automatic detecti…

2023 The Astrophysical Journal
IRIS 7
A geometric calibration of the tip of the red giant branch in the Milky Way using Gaia DR3
DOI: 10.1093/mnras/stad1500 Bibcode: 2023MNRAS.523.2283D

Lidman, C.; Flynn, C.; Dixon, M. +3 more

We use the latest parallaxes measurements from Gaia DR3 to obtain a geometric calibration of the tip of the red giant branch (TRGB) in Cousins I magnitudes as a standard candle for cosmology. We utilize the following surveys: SkyMapper DR3, APASS DR9, ATLAS Refcat2, and Gaia DR3 synthetic photometry to obtain multiple zero-point calibrations of th…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 7