Search Publications

SPLUS J210428.01-004934.2: An Ultra Metal-poor Star Identified from Narrowband Photometry
DOI: 10.3847/2041-8213/abf93d Bibcode: 2021ApJ...912L..32P

Lee, Young Sun; Placco, Vinicius M.; Roederer, Ian U. +6 more

We report on the discovery of SPLUS J210428.01-004934.2, an ultra metal-poor (UMP) star first identified from the narrowband photometry of the Southern Photometric Local Universe Survey (S-PLUS) Data Release 1, in the SDSS Stripe 82 region. Follow-up medium- and high-resolution spectroscopy (with Gemini South and Magellan-Clay, respectively) confi…

2021 The Astrophysical Journal
Gaia 36
Stellar Rotation of T Tauri Stars in the Orion Star-forming Complex
DOI: 10.3847/1538-4357/ac300a Bibcode: 2021ApJ...923..177S

Stassun, Keivan G.; Kounkel, Marina; Briceño, Cesar +14 more

We present a large-scale study of stellar rotation for T Tauri stars in the Orion star-forming complex. We use the projected rotational velocity ( $v\sin (i)$ vsin(i) ) estimations reported by the APOGEE-2 collaboration as well as individual masses and ages derived from the position of the stars in the HR diagram, considering Gaia-EDR3 parallaxes …

2021 The Astrophysical Journal
Gaia 36
Discovery of a Fast Iron Low-ionization Outflow in the Early Evolution of the Nearby Tidal Disruption Event AT 2019qiz
DOI: 10.3847/1538-4357/abf4c3 Bibcode: 2021ApJ...917....9H

Cenko, S. B.; Veilleux, S.; Filippenko, Alexei V. +16 more

We report the results of ultraviolet (UV) and optical photometric and spectroscopic analysis of the tidal disruption event (TDE) AT 2019qiz. Our follow-up observations started <10 days after the source began to brighten in the optical and lasted for a period of six months. Our late-time host-dominated spectrum indicates that the host galaxy lik…

2021 The Astrophysical Journal
eHST 36
Magellanic Mayhem: Metallicities and Motions
DOI: 10.3847/1538-4357/abd4e4 Bibcode: 2021ApJ...909..150G

Evans, N. W.; Belokurov, V.; Grady, J.

We assemble a catalog of Magellanic Cloud red giants from Data Release 2 of the Gaia mission and, utilizing machine-learning methods, obtain photometric metallicity estimates for them. In doing so, we are able to chemically map the entirety of the Magellanic System at once. Our maps reveal a plethora of substructure within our red giant sample, wi…

2021 The Astrophysical Journal
Gaia 35
From Pseudostreamer Jets to Coronal Mass Ejections: Observations of the Breakout Continuum
DOI: 10.3847/1538-4357/abca8b Bibcode: 2021ApJ...907...41K

Antiochos, Spiro K.; Lynch, Benjamin J.; Kumar, Pankaj +3 more

The magnetic breakout model, in which reconnection in the corona leads to destabilization of a filament channel, explains numerous features of eruptive solar events, from small-scale jets to global-scale coronal mass ejections (CMEs). The underlying multipolar topology, pre-eruption activities, and sequence of magnetic-reconnection onsets (first b…

2021 The Astrophysical Journal
Hinode SOHO 35
Reconstructing the Extreme Ultraviolet Emission of Cool Dwarfs Using Differential Emission Measure Polynomials
DOI: 10.3847/1538-4357/abeaaf Bibcode: 2021ApJ...913...40D

Loyd, R. O. Parke; Kowalski, Adam F.; Redfield, Seth +16 more

Characterizing the atmospheres of planets orbiting M dwarfs requires understanding the spectral energy distributions of M dwarfs over planetary lifetimes. Surveys like MUSCLES, HAZMAT, and FUMES have collected multiwavelength spectra across the spectral type's range of Teff and activity, but the extreme ultraviolet (EUV, 100-912 Å) flux…

2021 The Astrophysical Journal
eHST 35
RR Lyrae Variables in Messier 53: Near-infrared Period-Luminosity Relations and the Calibration Using Gaia Early Data Release 3
DOI: 10.3847/1538-4357/abdf48 Bibcode: 2021ApJ...909..200B

Herczeg, Gregory J.; de Grijs, Richard; Marconi, Marcella +6 more

We present new near-infrared, JHKs, period-luminosity relations (PLRs) for RR Lyrae variables in the Messier 53 (M53 or NGC 5024) globular cluster. Multi-epoch JHKs observations, obtained with the WIRCam instrument on the 3.6 m Canada-France-Hawaii Telescope, are used for the first time to estimate precise mean magnitudes for…

2021 The Astrophysical Journal
Gaia 35
Evidence for an MHD Disk Wind via Optical Forbidden Line Spectroastrometry
DOI: 10.3847/1538-4357/abf55e Bibcode: 2021ApJ...913...43W

Pascucci, I.; Sterzik, M. F.; Alexander, R. D. +4 more

Spectroastrometry is used to investigate the low-velocity component (LVC) of the optical forbidden emission from the T Tauri stars RU Lupi and AS 205 N. Both stars also have high-velocity forbidden emission, which is tracing a jet. For AS 205 N, analysis reveals a complicated outflow system. For RU Lupi, the [O I] λ6300 and [S II]λλ6716,6731 LV na…

2021 The Astrophysical Journal
Gaia 35
Probing Kilonova Ejecta Properties Using a Catalog of Short Gamma-Ray Burst Observations
DOI: 10.3847/1538-4357/ac04b4 Bibcode: 2021ApJ...916...89R

Berger, E.; Smith, N.; Chornock, R. +11 more

The discovery of GW170817 and GRB 170817A in tandem with AT 2017gfo cemented the connection between neutron star mergers, short gamma-ray bursts (GRBs), and kilonovae. To investigate short GRB observations in the context of diverse kilonova behavior, we present a comprehensive optical and near-IR catalog of 85 bursts discovered over 2005-2020 on t…

2021 The Astrophysical Journal
INTEGRAL eHST 35
First Simultaneous In Situ Measurements of a Coronal Mass Ejection by Parker Solar Probe and STEREO-A
DOI: 10.3847/1538-4357/ac0821 Bibcode: 2021ApJ...916...94W

Lugaz, Noé; Scolini, Camilla; Galvin, Antoinette B. +1 more

We present the first Parker Solar Probe mission (PSP)-observed coronal mass ejection (CME) that hits a second spacecraft before the end of the PSP encounter, providing an excellent opportunity to study short-term CME evolution. The CME was launched from the Sun on 2019 October 10 and was measured in situ at PSP on 2019 October 13 and at STEREO-A o…

2021 The Astrophysical Journal
SOHO 34