Search Publications

A Multiwavelength Study of the Sgr B Region: Contiguous Cloud-Cloud Collisions Triggering Widespread Star Formation Events?
DOI: 10.3847/1538-4357/ac674f Bibcode: 2022ApJ...931..155E

Fukui, Yasuo; Enokiya, Rei

The Sgr B region, including Sgr B1 and Sgr B2, is one of the most active star-forming regions in the Galaxy. Hasegawa et al. originally proposed that Sgr B2 was formed by a cloud-cloud collision (CCC) between two clouds with velocities of ~45 km s-1 and ~75 km s-1. However, some recent observational studies conflict with this…

2022 The Astrophysical Journal
Herschel 5
Call and Response: A Time-resolved Study of Chromospheric Evaporation in a Large Solar Flare
DOI: 10.3847/1538-4357/ac87a9 Bibcode: 2022ApJ...936...85S

Milligan, Ryan O.; McAteer, R. T. James; Sellers, Sean G.

We studied an X1.6 solar flare produced by NOAA Active Region 12602 on 2014 October 22. The entirety of this event was covered by RHESSI, IRIS, and Hinode/EIS, allowing analysis of the chromospheric response to a nonthermal electron driver. We derived the energy contained in nonthermal electrons via RHESSI spectral fitting and linked the time-depe…

2022 The Astrophysical Journal
Hinode IRIS 5
The Effect of Light Deflection by Solar System Objects on High-precision Square Kilometre Array Astrometry
DOI: 10.3847/1538-4357/ac8df8 Bibcode: 2022ApJ...938...58L

Xu, Ye; Hao, Chaojie; Li, Yingjie +4 more

We have computed the deflection angles caused by 195 objects in the solar system, including 177 satellites, and eight asteroids; 21 satellites and six asteroids can bend light from distant compact extragalactic sources by more than 0.1 µas, and 14 satellites, and the asteroid Ceres can deflect light by more than 1.0 µas. We calculated …

2022 The Astrophysical Journal
Gaia 5
Detection of a Broad 8 µm UIR Feature in the Mid-infrared Spectrum of WR 125 Observed with Subaru/COMICS
DOI: 10.3847/1538-4357/ac63bd Bibcode: 2022ApJ...930..116E

Onaka, Takashi; Sakon, Itsuki; Williams, Peredur M. +3 more

We present the detection of a broad 8 µm feature in newly formed dust around the carbon-rich Wolf-Rayet (WC) binary WR 125 from N-band low-resolution (NL; R ~ 250) spectroscopy between 7.3 and 13.6 µm and N-band (11.7 µm) and Q-band (18.8 µm) imaging with Subaru/COMICS in 2019 October. WR 125 is a colliding-wind binary (WC7…

2022 The Astrophysical Journal
AKARI ISO 5
Testing Lyα Emission-line Reconstruction Routines at Multiple Velocities in One System
DOI: 10.3847/1538-4357/ac87a8 Bibcode: 2022ApJ...936..189W

Redfield, Seth; Drake, Jeremy J.; France, Kevin +6 more

The 1215.67 Å H I Lyα emission line dominates the ultraviolet flux of low-mass stars, including the majority of known exoplanet hosts. Unfortunately, strong attenuation by the interstellar medium (ISM) obscures the line core in most stars, requiring the intrinsic Lyα flux to be reconstructed based on fits to the line wings. We present a test of th…

2022 The Astrophysical Journal
Gaia eHST 5
Direct Far-infrared Metal Abundances (FIRA). I. M101
DOI: 10.3847/1538-4357/ac3b4f Bibcode: 2022ApJ...925..194L

Smith, J. D.; Groves, B.; Linden, S. T. +12 more

Accurately determining gas-phase metal abundances within galaxies is critical as metals strongly affect the physics of the interstellar medium. To date, the vast majority of widely used gas-phase abundance indicators rely on emission from bright optical lines, whose emissivities are highly sensitive to the electron temperature. Alternatively, dire…

2022 The Astrophysical Journal
Herschel 5
A Molecular Gas Ring Hidden in the Sombrero Galaxy
DOI: 10.3847/1538-4357/ac9d8f Bibcode: 2022ApJ...941...47S

Fadda, Dario; Sutter, Jessica

We present Herschel, ALMA, and MUSE observations of the molecular ring of Messier 104, also known as the Sombrero galaxy. These previously unpublished archival data shed new light on the content of the interstellar medium of M104. In particular, molecular hydrogen measured by CO emission and dust measured by far-infrared light are uniformly distri…

2022 The Astrophysical Journal
Herschel 5
Unresolved z 8 Point Sources and Their Impact on the Bright End of the Galaxy Luminosity Function
DOI: 10.3847/1538-4357/ac8874 Bibcode: 2022ApJ...936..167I

Stiavelli, Massimo; Treu, Tommaso; Trenti, Michele +7 more

The distribution and properties of the first galaxies and quasars are critical pieces of the puzzle in understanding galaxy evolution and cosmic reionization. Previous studies have often excluded unresolved sources as potential low-redshift interlopers. We combine broadband color and photometric redshift analysis with morphological selections to i…

2022 The Astrophysical Journal
eHST 5
Yellow Post-asymptotic-giant-branch Stars as Standard Candles. I. Calibration of the Luminosity Function in Galactic Globular Clusters
DOI: 10.3847/1538-4357/ac674d Bibcode: 2022ApJ...930..145C

Bond, Howard E.; Ciardullo, Robin; Siegel, Michael H. +1 more

We use the results of a survey for low-surface-gravity stars in Galactic (and LMC) globular clusters to show that "yellow" post-asymptotic-branch (yPAGB) stars are likely to be excellent extragalactic standard candles, capable of producing distances to early-type galaxies that are accurate to a couple of percent. We show that the mean bolometric m…

2022 The Astrophysical Journal
Gaia 5
A 4 kpc Molecular Gas Lane in Cygnus A
DOI: 10.3847/1538-4357/ac8f45 Bibcode: 2022ApJ...937..106C

Nyland, Kristina; Decarli, Roberto; Perley, Daniel A. +4 more

We present the discovery of a 4 kpc molecular gas lane in the Cygnus A host galaxy, using Atacama Large Millimeter/submillimeter Array CO 2-1 observations. The gas lane is oriented roughly perpendicular to the projected radio jet axis. The CO emission generally follows the clumpy dust lanes seen in Hubble Space Telescope I-band images. The total m…

2022 The Astrophysical Journal
eHST 5