Search Publications

Unusual Galactic H II Regions at the Intersection of the Central Molecular Zone and the Far Dust Lane
DOI: 10.3847/1538-4357/abadf6 Bibcode: 2020ApJ...901...51A

Heywood, I.; Ginsburg, Adam; Glover, Simon C. O. +7 more

Sgr E is a massive star formation complex found toward the Galactic center that consists of numerous discrete, compact H II regions. It is located at the intersection between the central molecular zone (CMZ) and the far dust lane of the Galactic bar, similar to "hot spots" seen in external galaxies. Compared with other Galactic star formation comp…

2020 The Astrophysical Journal
Herschel 12
Toward Early-type Eclipsing Binaries as Extragalactic Milestones. II. NLTE Spectral Analysis and Stellar Parameters of the Detached O-type System OGLE-LMC-ECL-06782 in the LMC
DOI: 10.3847/1538-4357/ab6bd0 Bibcode: 2020ApJ...890..137T

Kudritzki, Rolf-Peter; Urbaneja, Miguel A.; Gieren, Wolfgang +5 more

We combine the NLTE spectral analysis of the detached O-type eclipsing binary OGLE-LMC-ECL-06782 with the analysis of the radial velocity curve and light curve to measure an independent distance to the Large Magellanic Cloud (LMC). In our spectral analysis we study composite spectra of the system at quadrature and use the information from radial v…

2020 The Astrophysical Journal
Gaia 12
The Three Young Nuclear Super Star Clusters in NGC 5253
DOI: 10.3847/1538-4357/ab8f94 Bibcode: 2020ApJ...896...84S

Smith, Linda J.; Sabbi, Elena; Ryon, Jenna +1 more

The blue compact dwarf galaxy NGC 5253 hosts a very young central starburst. The center contains intense radio thermal emission from a massive ultracompact H II region (or supernebula) and two massive and very young super star clusters (SSCs), which are seen at optical and infrared wavelengths. The spatial correspondence between these three object…

2020 The Astrophysical Journal
Gaia eHST 12
Fast and Wide CMEs without Observed >20 MeV Protons
DOI: 10.3847/1538-4357/ab64e1 Bibcode: 2020ApJ...889...92L

Thompson, B. J.; Lario, D.; Krupar, V. +6 more

Statistical studies have found a close association between large solar energetic particle (SEP) events and fast and wide coronal mass ejections (CMEs). However, not all fast and wide CMEs have an associated SEP event. From the Coordinated Data Analysis Web catalog of CMEs observed by the Solar and Heliospheric Observatory (SOHO) between 2009 Janua…

2020 The Astrophysical Journal
SOHO 12
Secular Extragalactic Parallax: Measurement Methods and Predictions for Gaia
DOI: 10.3847/1538-4357/ab6f00 Bibcode: 2020ApJ...890..146P

Darling, Jeremy; Paine, Jennie; Graziani, Romain +1 more

Secular extragalactic parallax caused by the solar system's velocity relative to the cosmic microwave background rest frame may be observable as a dipole proper motion field with amplitude 78 µas yr-1 Mpc. Nearby galaxies also exhibit proper motions caused by their transverse peculiar velocities that prevent detection of secular p…

2020 The Astrophysical Journal
Gaia 12
Study of the Decay Rates of the Umbral Area of Sunspot Groups Using a High-resolution Database
DOI: 10.3847/1538-4357/ab7898 Bibcode: 2020ApJ...892..107M

Muraközy, Judit

The emergence and decay of the sunspot groups are important components of the solar dynamo models. There are two different types of studies on the evolution of active regions. One of them is based on fewer data with higher spatial resolution, the other one uses more data with lower spatial resolution. The input data of the present study allow the …

2020 The Astrophysical Journal
SOHO 12
The Space Environment and Atmospheric Joule Heating of the Habitable Zone Exoplanet TOI 700 d
DOI: 10.3847/1538-4357/ab9637 Bibcode: 2020ApJ...897..101C

Drake, Jeremy J.; Garraffo, C.; Alvarado-Gómez, J. D. +4 more

We investigate the space environment conditions near the Earth-size planet TOI 700 d using a set of numerical models for the stellar corona and wind, the planetary magnetosphere, and the planetary ionosphere. We drive our simulations using a scaled-down stellar input and a scaled-up solar input in order to obtain two independent solutions. We find…

2020 The Astrophysical Journal
Ulysses 12
Infrared Properties of Asymptotic Giant Branch Stars in Our Galaxy and the Magellanic Clouds
DOI: 10.3847/1538-4357/ab6609 Bibcode: 2020ApJ...891...43S

Suh, Kyung-Won

We investigate the infrared properties of asymptotic giant branch (AGB) stars in our Galaxy and the Magellanic Clouds using various infrared observational data and theoretical models. We use catalogs for the sample of 4996 AGB stars in our Galaxy and about 39,000 AGB stars in the Magellanic Clouds from the available literature. For each object in …

2020 The Astrophysical Journal
AKARI 12
Cosmological 3D H I Gas Map with HETDEX Lyα Emitters and eBOSS QSOs at z = 2: IGM-Galaxy/QSO Connection and a ∼40 Mpc Scale Giant H II Bubble Candidate
DOI: 10.3847/1538-4357/abb81b Bibcode: 2020ApJ...903...24M

Ono, Yoshiaki; Ouchi, Masami; Finkelstein, Steven L. +20 more

We present cosmological (30-400 Mpc) distributions of neutral hydrogen (H I) in the intergalactic medium (IGM) traced by Lyα emitters (LAEs) and QSOs at z = 2.1-2.5, selected with the data of the ongoing Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) and the eBOSS survey. Motivated by a previous study of Mukae et al., we investigate spatia…

2020 The Astrophysical Journal
eHST 12
Soft X-Ray Observations of Quiescent Solar Active Regions Using the Novel Dual-zone Aperture X-Ray Solar Spectrometer
DOI: 10.3847/1538-4357/abba2a Bibcode: 2020ApJ...904...20S

Woods, Thomas N.; Caspi, Amir; Mason, James Paul +3 more

The Dual-zone Aperture X-ray Solar Spectrometer (DAXSS) was flown on 2018 June 18 on the NASA 36.336 sounding rocket flight and obtained the highest resolution to date for solar soft X-ray (SXR) spectra over a broad energy range. This observation was during a time with quiescent (nonflaring) small active regions on the solar disk and when the 10.7…

2020 The Astrophysical Journal
Hinode 12