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Chandra, NuSTAR, and Optical Observations of the Cataclysmic Variables IGR J17528-2022 and IGR J20063+3641
DOI: 10.3847/1538-4357/abfa96 Bibcode: 2021ApJ...914...85H

Mori, Kaya; Thorstensen, John R.; Halpern, Jules P. +5 more

We report on Chandra, NuSTAR, and MDM observations of two International Gamma-ray Astrophysics Laboratory (INTEGRAL) sources, namely IGR J17528-2022 and IGR J20063+3641. IGR J17528-2022 is an unidentified INTEGRAL source, while IGR J20063+3641 was recently identified as a magnetic cataclysmic variable (mCV) by Halpern et al. The Chandra observatio…

2021 The Astrophysical Journal
Gaia 9
A Giant Loop of Ionized Gas Emerging from the Tumultuous Central Region of IC 5063
DOI: 10.3847/1538-4357/ac0976 Bibcode: 2021ApJ...917...85M

Ho, Luis C.; Elvis, Martin; Fischer, Travis C. +6 more

The biconical radiation pattern extending from an active galactic nucleus (AGN) may strongly photoionize the circumnuclear interstellar medium (ISM) and stimulate emission from the narrow-line region (NLR). Observations of the NLR may provide clues to the structure of dense material that preferentially obscures the bicone at certain angles, and ma…

2021 The Astrophysical Journal
Gaia eHST 9
FOXSI-2 Solar Microflares. II. Hard X-ray Imaging Spectroscopy and Flare Energetics
DOI: 10.3847/1538-4357/abf145 Bibcode: 2021ApJ...913...15V

Krucker, Säm; Ryan, Daniel F.; Musset, Sophie +7 more

We study the nature of energy release and transfer for two sub-A class solar microflares observed during the second Focusing Optics X-ray Solar Imager (FOXSI-2) sounding rocket flight on 2014 December 11. FOXSI is the first solar-dedicated instrument to utilize focusing optics to image the Sun in the hard X-ray (HXR) regime, sensitive to energies …

2021 The Astrophysical Journal
IRIS 9
Implications of Increased Central Mass Surface Densities for the Quenching of Low-mass Galaxies
DOI: 10.3847/1538-4357/abf115 Bibcode: 2021ApJ...914....7G

Papovich, Casey; Pérez-González, Pablo G.; Bell, Eric F. +12 more

We use the Cosmic Assembly Deep Near-infrared Extragalactic Legacy Survey data to study the relationship between quenching and the stellar mass surface density within the central radius of 1 kpc (Σ1) of low-mass galaxies (stellar mass M* ≲ 109.5 M) at 0.5 ≤ z < 1.5. Our sample is mass complete down t…

2021 The Astrophysical Journal
eHST 9
The Characterization of the Dust Content in the Ring Around Sz 91: Indications of Planetesimal Formation?
DOI: 10.3847/1538-4357/ac21d0 Bibcode: 2021ApJ...923..128M

Palau, Aina; Carrasco-González, Carlos; Olofsson, Johan +6 more

One of the most important questions in the field of planet formation is how millimeter- and centimeter-sized dust particles overcome radial drift and fragmentation barriers to form kilometer-sized planetesimals. ALMA observations of protoplanetary disks, in particular transition disks or disks with clear signs of substructures, can provide new con…

2021 The Astrophysical Journal
Gaia 9
A Preliminary Calibration of the JAGB Method Using Gaia EDR3
DOI: 10.3847/1538-4357/ac2f4c Bibcode: 2021ApJ...923..157L

Madore, Barry F.; Freedman, Wendy L.; Lee, Abigail J. +2 more

The recently developed J-region asymptotic giant branch (JAGB) method has extraordinary potential as an extragalactic standard candle, capable of calibrating the absolute magnitudes of locally accessible Type Ia supernovae, thereby leading to an independent determination of the Hubble constant. Using Gaia Early Data Release 3 (EDR3) parallaxes, we…

2021 The Astrophysical Journal
Gaia 9
Gas Infalling Motions in the Envelopes of Very Low Luminosity Objects
DOI: 10.3847/1538-4357/abe4d3 Bibcode: 2021ApJ...910..112K

Kim, Gwanjeong; Kim, Mi-Ryang; Lee, Chang Won +2 more

We present the results of a single-dish survey toward 95 very low luminosity objects (VeLLOs) in optically thick (HCN 1-0) and thin (N2H+ 1-0) lines performed for the purpose of understanding the physical processes of inward motions in the envelopes of the VeLLOs and characterizing their true nature. The normalized velocity d…

2021 The Astrophysical Journal
Herschel 9
The Stellar Initial Mass Function and Population Properties of M89 from Optical and NIR Spectroscopy: Addressing Biases in Spectral Index Analysis
DOI: 10.3847/1538-4357/ac11f9 Bibcode: 2021ApJ...920...93L

Freedman, Wendy L.; Feldmeier-Krause, A.; Lonoce, I.

The complexity of constraining the stellar initial mass function (IMF) in early-type galaxies cannot be overstated, given the necessity of very high signal-to-noise ratio (S/N) data and the difficulty of breaking the strong degeneracies that occur among several stellar population parameters, including age, metallicity, and elemental abundances. Wi…

2021 The Astrophysical Journal
eHST 9
NOEMA Redshift Measurements of Extremely Bright Submillimeter Galaxies near the GOODS-N
DOI: 10.3847/1538-4357/ac05c1 Bibcode: 2021ApJ...916...46J

Cowie, Lennox L.; Barger, Amy J.; Jones, Logan H. +1 more

We report spectroscopic redshift measurements for three bright submillimeter galaxies (SMGs) near the GOODS-N field, each with SCUBA-2 850 µm fluxes >10 mJy, using the Northern Extended Millimeter Array (NOEMA). Our molecular line-scan observations of these sources, which occupy an ~7 arcmin2 area outside of the Hubble Space Te…

2021 The Astrophysical Journal
Herschel 9
On the Possibility of Stellar Lenses in the Black Hole Candidate Microlensing Events MACHO-96-BLG-5 and MACHO-98-BLG-6
DOI: 10.3847/1538-4357/abee83 Bibcode: 2021ApJ...912..146A

Lu, Jessica R.; Abdurrahman, Fatima N.; Stephens, Haynes F.

Although stellar-mass black holes (BHs) are likely to be abundant in the Milky Way (N = 108-109), only 20 have been detected to date, all in accreting binary systems. Gravitational microlensing is a proposed technique to search for isolated BHs, which have not yet been detected. Two specific microlensing events, MACHO-1996-BL…

2021 The Astrophysical Journal
Gaia eHST 9