Search Publications

Toward Precision Cosmology with Improved PNLF Distances Using VLT-MUSEI. Methodology and Tests
DOI: 10.3847/1538-4357/ac02ca Bibcode: 2021ApJ...916...21R

Weilbacher, Peter M.; Roth, Martin M.; Ciardullo, Robin +3 more

The [O III] λ5007 planetary nebula luminosity function (PNLF) is an established distance indicator that has been used for more than 30 yr to measure the distances of galaxies out to ~15 Mpc. With the advent of the Multi-Unit Spectroscopic Explorer on the Very Large Telescope (MUSE) as an efficient wide-field integral-field spectrograph, the PNLF m…

2021 The Astrophysical Journal
eHST 27
Three K2 Campaigns Yield Rotation Periods for 1013 Stars in Praesepe
DOI: 10.3847/1538-4357/ac0c1e Bibcode: 2021ApJ...921..167R

Cargile, Phillip A.; Rampalli, Rayna; Law, Nicholas M. +8 more

We use three campaigns of K2 observations to complete the census of rotation in low-mass members of the benchmark, ≈670 Myr old open cluster Praesepe. We measure new rotation periods (P rot) for 220 ≲1.3 M Praesepe members and recovery periods for 97% (793/812) of the stars with a P rot in the literature. Of the …

2021 The Astrophysical Journal
Gaia 27
Formation of Phosphorus Monoxide (PO) in the Interstellar Medium: Insights from Quantum-chemical and Kinetic Calculations
DOI: 10.3847/1538-4357/ac1e94 Bibcode: 2021ApJ...922..169G

Jiménez-Serra, Izaskun; Roncero, Octavio; García de la Concepción, Juan +2 more

In recent years, phosphorus monoxide (PO), an important molecule for prebiotic chemistry, has been detected in star-forming regions and in the comet 67P/Churyumov-Gerasimenko. These studies have revealed that, in the interstellar medium (ISM), PO is systematically the most abundant P-bearing species, with abundances that are about one to three tim…

2021 The Astrophysical Journal
Rosetta 27
The Sloan Digital Sky Survey Reverberation Mapping Project: The MBH-Host Relations at 0.2 ≲ z ≲ 0.6 from Reverberation Mapping and Hubble Space Telescope Imaging
DOI: 10.3847/1538-4357/abc8e6 Bibcode: 2021ApJ...906..103L

Trump, Jonathan R.; Brandt, W. N.; Shen, Yue +10 more

We present the results of a pilot Hubble Space Telescope (HST) imaging study of the host galaxies of ten quasars from the Sloan Digital Sky Survey Reverberation Mapping (SDSS-RM) project. Probing more than an order of magnitude in black hole (BH) and stellar masses, our sample is the first statistical sample to study the BH-host correlations beyon…

2021 The Astrophysical Journal
eHST 27
On the Use of Field RR Lyrae As Galactic Probes: IV. New Insights Into and Around the Oosterhoff Dichotomy
DOI: 10.3847/1538-4357/ac1115 Bibcode: 2021ApJ...919..118F

Salaris, M.; Lemasle, B.; Zoccali, M. +30 more

We discuss the largest and most homogeneous spectroscopic data set of field RR Lyrae variables (RRLs) available to date. We estimated abundances using both high-resolution and low-resolution (ΔS method) spectra for fundamental (RRab) and first overtone (RRc) RRLs. The iron abundances for 7941 RRLs were supplemented with similar estimates that are …

2021 The Astrophysical Journal
Gaia 26
A Study of the Photometric and Spectroscopic Variations of the Prototypical FU Orionis-type Star V1057 Cyg
DOI: 10.3847/1538-4357/ac04b3 Bibcode: 2021ApJ...917...80S

Cseh, B.; Kriskovics, L.; Pál, A. +19 more

Among the low-mass pre-main sequence stars, a small group called FU Orionis-type objects (FUors) are notable for undergoing powerful accretion outbursts. V1057 Cyg, a classical example of an FUor, went into outburst around 1969-1970, after which it faded rapidly, making it the fastest-fading FUor known. Around 1995, a more rapid increase in fading…

2021 The Astrophysical Journal
Gaia Herschel ISO 26
Stellar Superflares Observed Simultaneously with Kepler and XMM-Newton
DOI: 10.3847/1538-4357/abf569 Bibcode: 2021ApJ...912...81K

Kolotkov, Dmitrii Y.; Kuznetsov, Alexey A.

Solar and stellar flares are powerful events that produce intense radiation across the electromagnetic spectrum. Multiwavelength observations are highly important for understanding the nature of flares, because different flare-related processes reveal themselves in different spectral ranges. To study the correlation between thermal and nonthermal …

2021 The Astrophysical Journal
XMM-Newton 26
Visual Explanation of a Deep Learning Solar Flare Forecast Model and Its Relationship to Physical Parameters
DOI: 10.3847/1538-4357/abdebe Bibcode: 2021ApJ...910....8Y

Moon, Yong-Jae; Lim, Daye; Lee, Harim +2 more

In this study, we present a visual explanation of a deep learning solar flare forecast model and its relationship to physical parameters of solar active regions (ARs). For this, we use full-disk magnetograms at 00:00 UT from the Solar and Heliospheric Observatory/Michelson Doppler Imager and the Solar Dynamics Observatory/Helioseismic and Magnetic…

2021 The Astrophysical Journal
SOHO 26
Evidence for a Cosmic-Ray Gradient in the IM Lup Protoplanetary Disk
DOI: 10.3847/1538-4357/abf09a Bibcode: 2021ApJ...912..136S

Seifert, Richard A.; Cleeves, L. Ilsedore; Adams, Fred C. +1 more

Protoplanetary disk evolution is strongly impacted by ionization from the central star and local environment, which collectively have been shown to drive chemical complexity and are expected to impact the transport of disk material. Nonetheless, ionization remains a poorly constrained input to many detailed modeling efforts. We use new and archiva…

2021 The Astrophysical Journal
Gaia 26
Dynamical Stellar Masses of Pre-main-sequence Stars in Lupus and Taurus Obtained with ALMA Surveys in Comparison with Stellar Evolutionary Models
DOI: 10.3847/1538-4357/abd24f Bibcode: 2021ApJ...908...46B

Koch, Patrick M.; Yen, Hsi-Wei; Testi, Leonardo +3 more

We analyzed archival molecular line data of pre-main-sequence (PMS) stars in the Lupus and Taurus star-forming regions obtained with ALMA surveys with an integration time of a few minutes per source. We stacked the data of 13CO and C18O (J = 2-1 and 3-2) and CN (N = 3-2, J = 7/2-5/2) lines to enhance the signal-to-noise ratio…

2021 The Astrophysical Journal
Gaia 26