Search Publications

Origin of Quasi-periodic Pulsation at the Base of a Kink-unstable Jet
DOI: 10.3847/1538-4357/acb058 Bibcode: 2023ApJ...945..113M

Srivastava, A. K.; Kayshap, Pradeep; Rajaguru, S. P. +3 more

We studied a blowout jet that occurred at the west limb of the Sun on 2014 August 29 using high-resolution imaging/spectroscopic observations provided by the Solar Dynamics Observatory/Atmospheric Imaging Assembly and the Interface Region Imaging Spectrograph. An inverse γ-shaped flux rope appeared before the jet-morphological indication of the on…

2023 The Astrophysical Journal
IRIS 7
Green Bank Telescope Discovery of the Redback Binary Millisecond Pulsar PSR J0212+5321
DOI: 10.3847/1538-4357/acdc23 Bibcode: 2023ApJ...952..150P

Perez, Karen I.; Bogdanov, Slavko; Halpern, Jules P. +1 more

We report the discovery of a 2.11 ms binary millisecond pulsar during a targeted search of the redback optical candidate coincident with the γ-ray source 3FGL J0212.5+5320 using the Robert C. Byrd Green Bank Telescope (GBT) with the Breakthrough Listen backend at L band. Over a seven month period, five pointings were made near inferior conjunction…

2023 The Astrophysical Journal
Gaia 7
ALMA High-frequency Long Baseline Campaign in 2021: Highest Angular Resolution Submillimeter Wave Images for the Carbon-rich Star R Lep
DOI: 10.3847/1538-4357/acf619 Bibcode: 2023ApJ...958...86A

Hirota, Akihiko; Hales, Antonio S.; Takahashi, Satoko +11 more

The Atacama Large Millimeter/submillimeter Array (ALMA) was used in 2021 to image the carbon-rich evolved star R Lep in Bands 8-10 (397-908 GHz) with baselines up to 16 km. The goal was to validate the calibration, using band-to-band (B2B) phase referencing with a close phase calibrator J0504-1512, 1.°2 from R Lep in this case, and the imaging pro…

2023 The Astrophysical Journal
Gaia 7
ALMA 1.1 mm Observations of a Conservative Sample of High-redshift Massive Quiescent Galaxies in SHELA
DOI: 10.3847/1538-4357/acd1e3 Bibcode: 2023ApJ...951...49C

Papovich, Casey; Finkelstein, Steven L.; Bagley, Micaela B. +11 more

We present a sample of 30 massive (log(M */M ) > 11) z = 3-5 quiescent galaxies selected from the Spitzer-HETDEX Exploratory Large Area (SHELA) Survey and observed at 1.1 mm with Atacama Large Millimeter/submillimeter Array (ALMA) Band 6 observations. These ALMA observations would detect even modest levels of dust-obscure…

2023 The Astrophysical Journal
Gaia 7
Discovery of the Exceptionally Short Period Ultracool Dwarf Binary LP 413-53AB
DOI: 10.3847/2041-8213/acba8c Bibcode: 2023ApJ...945L...6H

Burgasser, Adam J.; Hsu, Chih-Chun; Theissen, Christopher A.

We report the detection of large-amplitude, rapid radial velocity (RV) variations and line-splitting in high-resolution Keck/NIRSPEC spectra of the M9 dwarf LP 413-53. We attribute these features to binary motion. Analyzing data spanning 15 yr, we infer a preliminary orbital period of 0.7106156 ± 0.0000002 days, an eccentricity of 0.0088 ± 0.0017,…

2023 The Astrophysical Journal
Gaia 7
The Metallicity and Distance of Leo A from Blue Supergiants
DOI: 10.3847/1538-4357/acfc3d Bibcode: 2023ApJ...959...52U

Bresolin, Fabio; Kudritzki, Rolf-Peter; Urbaneja, Miguel A.

We have obtained high-quality spectra of blue supergiant candidates in the dwarf irregular galaxy Leo A with the Low Resolution Imaging Spectrometer at the Keck I telescope. From the quantitative analysis of seven B8-A0 stars, we derive a mean metallicity [Z] = -1.35 ± 0.08, in excellent agreement with the gas-phase chemical abundance. From the st…

2023 The Astrophysical Journal
eHST 7
Understanding the Relationship between Solar Coronal Abundances and F10.7 cm Radio Emission
DOI: 10.3847/1538-4357/acbc1b Bibcode: 2023ApJ...948..121T

Long, David M.; Brooks, David H.; Baker, Deborah +7 more

Sun-as-a-star coronal plasma composition, derived from full-Sun spectra, and the F10.7 radio flux (2.8 GHz) have been shown to be highly correlated (r = 0.88) during solar cycle 24. However, this correlation becomes nonlinear during increased solar magnetic activity. Here we use cotemporal, high spatial resolution, multiwavelength images of the Su…

2023 The Astrophysical Journal
Hinode 7
Infrared Ejecta and Cold Dust in the Young Supernova Remnant N132D
DOI: 10.3847/1538-4357/acc392 Bibcode: 2023ApJ...949...74R

Slavin, Jonathan D.; Rho, Jeonghee; Ravi, Aravind P. +1 more

We present Spitzer, Wide-field Infrared Survey Explorer (WISE), and Herschel observations of the young supernova remnant (SNR) N132D in the Large Magellanic Cloud, including 3-40 µm Spitzer Infrared Spectrograph (IRS) mapping, 12 µm WISE and 70, 100, 160, 250, 350, and 500 µm Herschel images. The high-velocity lines of [Ne II] at…

2023 The Astrophysical Journal
Herschel 7
Delayed Development of Cool Plasmas in X-Ray Flares from the Young Sun-like Star κ 1 Ceti
DOI: 10.3847/1538-4357/acae8b Bibcode: 2023ApJ...944..163H

Hamaguchi, Kenji; Toriumi, Shin; Arzoumanian, Zaven +3 more

The Neutron star Interior Composition Explorer (NICER) X-ray observatory observed two powerful X-ray flares equivalent to superflares from the nearby young solar-like star κ 1 Ceti in 2019. NICER follows each flare from the onset through the early decay, collecting over 30 counts s-1 near the peak, enabling a detailed spectra…

2023 The Astrophysical Journal
XMM-Newton 7
The Masses of Supernova Remnant Progenitors in M33
DOI: 10.3847/1538-4357/acc249 Bibcode: 2023ApJ...949...32K

Williams, Benjamin F.; Dolphin, Andrew; Dalcanton, Julianne J. +7 more

Using resolved optical stellar photometry from the Panchromatic Hubble Andromeda Treasury Triangulum Extended Region survey, we measured the star formation history near the position of 85 supernova remnants (SNRs) in M33. We constrained the progenitor masses for 60 of these SNRs, finding that the remaining 25 remnants had no local star formation i…

2023 The Astrophysical Journal
eHST 7