Search Publications

M17 MIR: A Massive Protostar with Multiple Accretion Outbursts
DOI: 10.3847/1538-4357/ac2151 Bibcode: 2021ApJ...922...90C

Chen, Zhiwei; Chen, Xuepeng; Haas, Martin +3 more

We report the discovery of a massive protostar M17 MIR embedded in a hot molecular core in M17. The multiwavelength data obtained during 1993-2019 show significant mid-IR (MIR) variations, which can be split into three stages: the decreasing phase during 1993.03-mid-2004, the quiescent phase from mid-2004 to mid-2010, and the rebrightening phase f…

2021 The Astrophysical Journal
Herschel ISO 26
Millimeter-sized Dust Grains Surviving the Water-sublimating Temperature in the Inner 10 au of the FU Ori Disk
DOI: 10.3847/1538-4357/ac31b9 Bibcode: 2021ApJ...923..270L

Chen, Wen Ping; Liu, Sheng-Yuan; Takami, Michihiro +11 more

Previous observations have shown that the ≲10 au, ≳400 K hot inner disk of the archetypal accretion outburst young stellar object, FU Ori, is dominated by viscous heating. To constrain dust properties in this region, we have performed radio observations toward this disk using the Karl G. Jansky Very Large Array in 2020 June-July, September, and No…

2021 The Astrophysical Journal
Gaia Herschel 26
Hinode/EIS Coronal Magnetic Field Measurements at the Onset of a C2 Flare
DOI: 10.3847/1538-4357/abf6d1 Bibcode: 2021ApJ...913....1L

Landi, E.; Li, W.; Hutton, R. +1 more

We study Hinode/EIS observations of an active region taken before, during, and after a small C2.0 flare in order to monitor the evolution of the magnetic field and its relation to the flare event. We find that while the flare left the active region itself unaltered, the event included a large magnetic field enhancement (MFE), which consisted of a …

2021 The Astrophysical Journal
Hinode 26
Global Distribution of the Solar Wind Speed Reconstructed from Improved Tomographic Analysis of Interplanetary Scintillation Observations between 1985 and 2019
DOI: 10.3847/1538-4357/ac1862 Bibcode: 2021ApJ...922...73T

Kojima, Masayoshi; Tokumaru, Munetoshi; Fujiki, Ken'ichi +1 more

Computer-assisted tomography (CAT) for interplanetary scintillation (IPS) observations enables the determination of the global distribution of solar wind speed. We compared solar wind speeds derived from the CAT analysis of IPS observations between 1985 and 2019 with in situ observations conducted by the near-Earth and Ulysses spacecraft. From thi…

2021 The Astrophysical Journal
Ulysses 26
Spectroscopy and Photometry of the Least Massive Type II Globular Clusters: NGC 1261 and NGC 6934
DOI: 10.3847/1538-4357/ac282c Bibcode: 2021ApJ...923...22M

Da Costa, G. S.; Milone, A. P.; Cordoni, G. +10 more

Recent work has revealed two classes of globular clusters (GCs), dubbed Type I and Type II. Type II GCs are characterized by both a blue and a red red giant branch composed of stars with different metallicities, often coupled with distinct abundances in the slow neutron-capture elements (s-elements). Here we continue the chemical tagging of Type I…

2021 The Astrophysical Journal
eHST 26
Resolving the Dust-to-Metals Ratio and CO-to-H2 Conversion Factor in the Nearby Universe
DOI: 10.3847/1538-4357/abceb6 Bibcode: 2021ApJ...907...29C

Sandstrom, Karin M.; Leroy, Adam K.; Schruba, Andreas +8 more

We investigate the relationship between the dust-to-metals ratio (D/M) and the local interstellar medium environment at ∼2 kpc resolution in five nearby galaxies: IC 342, M31, M33, M101, and NGC 628. A modified blackbody model with a broken power-law emissivity is used to model the dust emission from 100 to 500 µm observed by Herschel. We ut…

2021 The Astrophysical Journal
Herschel 26
Grain Growth in Escaping Atmospheres: Implications for the Radius Inflation of Super-Puffs
DOI: 10.3847/1538-4357/ac1516 Bibcode: 2021ApJ...920..124O

Ohno, Kazumasa; Tanaka, Yuki A.

Super-puffs-low-mass exoplanets with extremely low bulk density-are attractive targets for exploring their atmospheres and formation processes. Recent studies suggested that the large radii of super-puffs may be caused by atmospheric dust entrained in the escaping atmospheres. In this study, we investigate how the dust grows in escaping atmosphere…

2021 The Astrophysical Journal
eHST 26
Head-to-Toe Measurement of El Gordo: Improved Analysis of the Galaxy Cluster ACT-CL J0102-4915 with New Wide-field Hubble Space Telescope Imaging Data
DOI: 10.3847/1538-4357/ac294f Bibcode: 2021ApJ...923..101K

Sifón, Cristóbal; Hughes, John P.; Jee, M. James +6 more

We present an improved weak-lensing (WL) study of the high-z (z = 0.87) merging galaxy cluster ACT-CL J0102-4915 ("El Gordo") based on new wide-field Hubble Space Telescope imaging data. The new imaging data cover the ~3.5 × ~3.5 Mpc region centered on the cluster and enable us to detect WL signals beyond the virial radius, which was not possible …

2021 The Astrophysical Journal
eHST 26
Revisiting Dynamical Friction: The Role of Global Modes and Local Wakes
DOI: 10.3847/1538-4357/ac0627 Bibcode: 2021ApJ...916...55T

Babul, Arif; Quinn, Thomas R.; Mayer, Lucio +4 more

The orbital decay of a perturber within a larger system plays a key role in the dynamics of many astrophysical systems-from nuclear star clusters or globular clusters in galaxies, to massive black holes in galactic nuclei, to dwarf galaxy satellites within the dark matter halos of more massive galaxies. For many decades, there have been various at…

2021 The Astrophysical Journal
Gaia 26
R-process-rich Stellar Streams in the Milky Way
DOI: 10.3847/1538-4357/abea1a Bibcode: 2021ApJ...912...52G

Roederer, Ian U.; Frebel, Anna; Ji, Alexander P. +3 more

We present high-resolution Magellan/MIKE spectra of 22 bright (9 < V < 13.5) metal-poor stars (-3.18 < [Fe/H] < -1.37) in three different stellar streams, the Helmi debris stream, the Helmi trail stream, and the ω Centauri progenitor stream. We augment our Helmi debris sample with results for 10 stars by Roederer et al. for a total of …

2021 The Astrophysical Journal
Gaia 25