Search Publications

Network Jets as the Driver of Counter-streaming Flows in a Solar Filament/Filament Channel
DOI: 10.3847/2041-8213/ab9ac1 Bibcode: 2020ApJ...897L...2P

Tiwari, Sanjiv K.; Panesar, Navdeep K.; Moore, Ronald L. +1 more

Counter-streaming flows in a small (100″ long) solar filament/filament channel are directly observed in high-resolution Solar Dynamics Observatory (SDO)/Atmospheric Imaging Assembly (AIA) extreme-ultraviolet (EUV) images of a region of enhanced magnetic network. We combine images from SDO/AIA, SDO/Helioseismic and Magnetic Imager (HMI), and the In…

2020 The Astrophysical Journal
IRIS 22
Scaling K2. II. Assembly of a Fully Automated C5 Planet Candidate Catalog Using EDI-Vetter
DOI: 10.3847/1538-3881/ab7448 Bibcode: 2020AJ....159..154Z

Schlieder, Joshua E.; Petigura, Erik A.; Crossfield, Ian J. M. +5 more

We present a uniform transiting exoplanet candidate list for Campaign 5 of the K2 mission. This catalog contains 75 planets with seven multi-planet systems (five double, one triple, and one quadruple planet system). Within the range of our search, we find eight previously undetected candidates, with the remaining 67 candidates overlapping 51% of t…

2020 The Astronomical Journal
Gaia 22
Space weathering by simulated micrometeorite bombardment on natural olivine and pyroxene: A coordinated IR and TEM study
DOI: 10.1016/j.epsl.2019.115884 Bibcode: 2020E&PSL.53015884W

Hiesinger, Harald; Helbert, Jörn; Weber, Iris +9 more

We studied space-weathering effects caused by micrometeorite bombardment simulated by pulsed intense infrared laser, generating ∼15 mJ per pulse in high vacuum. For our investigation, we selected a natural olivine (San Carlos olivine (Fo91)) and a natural pyroxene (Bamble orthopyroxene (En87)) as important rock forming minera…

2020 Earth and Planetary Science Letters
BepiColombo 22
The CGM at Cosmic Noon with KCWI: Outflows from a Star-forming Galaxy at z = 2.071
DOI: 10.3847/1538-4357/abc561 Bibcode: 2020ApJ...904..164N

Kacprzak, Glenn G.; Churchill, Christopher W.; Davé, Romeel +3 more

We present the first results from our "CGM at Cosmic Noon with KCWI" program to study gas flows in the circumgalactic medium (CGM) at z = 2-3. Combining the power of a high-resolution VLT/UVES quasar spectrum, a Hubble Space Telescope/Advanced Camera for Surveys image, and integral field spectroscopy with Keck/KCWI (Keck Cosmic Web Imager), we det…

2020 The Astrophysical Journal
eHST 22
LBT transmission spectroscopy of HAT-P-12b. Confirmation of a cloudy atmosphere with no significant alkali features
DOI: 10.1051/0004-6361/201937265 Bibcode: 2020A&A...642A..98Y

Mallonn, M.; Reiners, A.; Apai, D. +10 more

The hot sub-Saturn-mass exoplanet HAT-P-12b is an ideal target for transmission spectroscopy because of its inflated radius. We observed one transit of the planet with the multi-object double spectrograph (MODS) on the Large Binocular Telescope (LBT) with the binocular mode and obtained an atmosphere transmission spectrum with a wavelength coverag…

2020 Astronomy and Astrophysics
eHST 22
An Observationally Constrained Analytical Model for Predicting the Magnetic Field Vectors of Interplanetary Coronal Mass Ejections at 1 au
DOI: 10.3847/1538-4357/ab5fd7 Bibcode: 2020ApJ...888..121S

Gopalswamy, Nat; Srivastava, Nandita; Sarkar, Ranadeep

We report on an observationally constrained analytical model, the INterplanetary Flux ROpe Simulator (INFROS), for predicting the magnetic field vectors of coronal mass ejections (CMEs) in the interplanetary medium. The main architecture of INFROS involves using the near-Sun flux rope properties obtained from the observational parameters that are …

2020 The Astrophysical Journal
SOHO 22
A radio polarimetric study to disentangle AGN activity and star formation in Seyfert galaxies
DOI: 10.1093/mnras/staa2473 Bibcode: 2020MNRAS.499..334S

O'Dea, C. P.; Baum, S. A.; Kharb, P. +2 more

To understand the origin of radio emission in radio-quiet active galactic nucleus (AGN) and differentiate between the contributions from star formation, AGN accretion, and jets, we have observed a nearby sample of Seyfert galaxies along with a comparison sample of starburst galaxies using the Expanded Very Large Array (EVLA) in full-polarization m…

2020 Monthly Notices of the Royal Astronomical Society
eHST 22
The Most Metal-poor Stars in the Inner Bulge
DOI: 10.3847/1538-3881/aba948 Bibcode: 2020AJ....160..173R

Casey, Andrew R.; Ji, Alexander P.; Reggiani, Henrique +1 more

The bulge is the oldest component of the Milky Way. Since numerous simulations of Milky Way formation have predicted that the oldest stars at a given metallicity are found on tightly bound orbits, the Galaxy's oldest stars are likely metal-poor stars in the inner bulge with small apocenters (i.e., Rapo ≲ 4 kpc). In the past, stars with …

2020 The Astronomical Journal
Gaia 22
A stellar census in globular clusters with MUSE. Extending the CaT-metallicity relation below the horizontal branch and applying it to multiple populations
DOI: 10.1051/0004-6361/201936508 Bibcode: 2020A&A...635A.114H

Brinchmann, Jarle; Weilbacher, Peter M.; Kamann, Sebastian +7 more


Aims: We use the spectra of more than 30 000 red giant branch (RGB) stars in 25 globular clusters (GC), obtained within the MUSE survey of Galactic globular clusters, to calibrate the Ca II triplet metallicity relation and derive metallicities for all individual stars. We investigate the overall metallicity distributions as well as those of t…

2020 Astronomy and Astrophysics
eHST 22
Discovery and Rapid Follow-up Observations of the Unusual Type II SN 2018ivc in NGC 1068
DOI: 10.3847/1538-4357/ab8945 Bibcode: 2020ApJ...895...31B

Fox, O. D.; Zhang, X.; Reichart, D. E. +46 more

We present the discovery and high-cadence follow-up observations of SN 2018ivc, an unusual SNe II that exploded in NGC 1068 (D = 10.1 Mpc). The light curve of SN 2018ivc declines piecewise-linearly, changing slope frequently, with four clear slope changes in the first 30 days of evolution. This rapidly changing light curve indicates that interacti…

2020 The Astrophysical Journal
eHST 22