Search Publications

The Origin of the Doppler Flip in HD 100546: A Large-scale Spiral Arm Generated by an Inner Binary Companion
DOI: 10.3847/2041-8213/ac85ed Bibcode: 2022ApJ...936L...4N

Ginski, Christian; Pinte, Christophe; Rosotti, Giovanni +9 more

Companions at subarcsecond separation from young stars are difficult to image. However, their presence can be inferred from the perturbations they create in the dust and gas of protoplanetary disks. Here we present a new interpretation of SPHERE polarized observations that reveal the previously detected inner spiral in the disk of HD 100546. The s…

2022 The Astrophysical Journal
Gaia 13
Linking Small-scale Solar Wind Properties with Large-scale Coronal Source Regions through Joint Parker Solar Probe-Metis/Solar Orbiter Observations
DOI: 10.3847/1538-4357/ac8103 Bibcode: 2022ApJ...935..112T

Telloni, Daniele; Zank, Gary P.; Adhikari, Laxman +92 more

The solar wind measured in situ by Parker Solar Probe in the very inner heliosphere is studied in combination with the remote-sensing observation of the coronal source region provided by the METIS coronagraph aboard Solar Orbiter. The coronal outflows observed near the ecliptic by Metis on 2021 January 17 at 16:30 UT, between 3.5 and 6.3 R ⊙<…

2022 The Astrophysical Journal
SolarOrbiter 13
Disconnecting the Dots: Re-examining the Nature of Stellar "Strings" in the Milky Way
DOI: 10.3847/1538-4357/ac898c Bibcode: 2022ApJ...936..160Z

Peek, J. E. G.; Zucker, Catherine; Loebman, Sarah

Recent analyses of Gaia data have resulted in the identification of new stellar structures, including a new class of extended stellar filaments called stellar "strings," first proposed by Kounkel & Covey. We explore the spatial, kinematic, and chemical composition of strings to demonstrate that these newfound structures are largely inconsisten…

2022 The Astrophysical Journal
Gaia 13
The X-Ray Luminosity Function Evolution of Quasars and the Correlation between the X-Ray and Ultraviolet Luminosities
DOI: 10.3847/1538-4357/ac6f06 Bibcode: 2022ApJ...932..111S

Singal, J.; Mutchnick, S.; Petrosian, V.

We explore the evolution of the X-ray luminosity function of quasars and the intrinsic correlation between the X-ray and 2500 Å ultraviolet luminosities, utilizing techniques verified in previous works and a sample of over 4000 quasars detected with Chandra and XMM-Newton in the range 0 < z < 5. We find that quasars have undergone significan…

2022 The Astrophysical Journal
XMM-Newton 13
Deep XMM-Newton Observations of an X-ray Weak Broad Absorption Line Quasar at z = 6.5
DOI: 10.3847/2041-8213/ac45f2 Bibcode: 2022ApJ...924L..25Y

Fan, Xiaohui; Keeton, Charles R.; Walter, Fabian +14 more

We report X-ray observations of the most distant known gravitationally lensed quasar, J0439+1634 at z = 6.52, which is also a broad absorption line (BAL) quasar, using the XMM-Newton Observatory. With a 130 ks exposure, the quasar is significantly detected as a point source at the optical position with a total of ${358}_{-19}^{+19}$ net counts usi…

2022 The Astrophysical Journal
XMM-Newton 13
The "Singular" Behavior of the Solar Wind Scaling Features during Parker Solar Probe-BepiColombo Radial Alignment
DOI: 10.3847/1538-4357/ac478d Bibcode: 2022ApJ...926..174A

Richter, Ingo; Auster, Hans-Ulrich; Hadid, Lina Z. +4 more

At the end of 2020 September, the Parker Solar Probe (PSP) and BepiColombo were radially aligned: PSP was orbiting near 0.17 au and BepiColombo near 0.6 au. This geometry is of particular interest for investigating the evolution of solar wind properties at different heliocentric distances by observing the same solar wind plasma parcels. In this wo…

2022 The Astrophysical Journal
BepiColombo 13
A Partial Filament Eruption in Three Steps Induced by External Magnetic Reconnection
DOI: 10.3847/1538-4357/ac4fbe Bibcode: 2022ApJ...929...85D

Xu, Zhe; Li, Leping; Zhang, Qingmin +6 more

We present an investigation of partial filament eruption on 2012 June 17 in the active region NOAA 11504. For the first time, we observed the vertical splitting process during the partial eruption with high-resolution narrowband images at 10830 Å. The active filament was rooted in a small δ-sunspot of the active region. Particularly, it underwent …

2022 The Astrophysical Journal
SOHO 13
MARS: A New Maximum-entropy-regularized Strong Lensing Mass Reconstruction Method
DOI: 10.3847/1538-4357/ac69df Bibcode: 2022ApJ...931..127C

Jee, M. James; Cha, Sangjun

Free-form strong-lensing (SL) mass reconstructions typically suffer from overfitting, which manifests itself as false-positive small-scale fluctuations. We present a new free-form MAximum-entropy ReconStruction (MARS) method without the assumption that light traces mass (LTM). The MARS algorithm enables us to achieve excellent convergence in sourc…

2022 The Astrophysical Journal
eHST 13
The Nascent Milliquasar VT J154843.06+220812.6: Tidal Disruption Event or Extreme Accretion State Change?
DOI: 10.3847/1538-4357/ac5e29 Bibcode: 2022ApJ...929..184S

Hallinan, Gregg; Graham, Matthew; Lu, Wenbin +5 more

We present a detailed multiwavelength follow-up of the nuclear radio flare VT J154843.06+220812.6, hereafter VT J1548. VT J1548 was selected as a ~1 mJy radio flare in 3 GHz observations from the Very Large Array Sky Survey. It is located in the nucleus of a low-mass ( $\mathrm{log}{M}_{\mathrm{BH}}/{M}_{\odot }\sim 6$ ) host galaxy with weak or n…

2022 The Astrophysical Journal
XMM-Newton 13
A Panchromatic Study of Massive Stars in the Extremely Metal-poor Local Group Dwarf Galaxy Leo A
DOI: 10.3847/1538-4357/aca295 Bibcode: 2022ApJ...941..206G

McQuinn, Kristen B. W.; Williams, Benjamin F.; Choi, Yumi +17 more

We characterize massive stars (M > 8 M ) in the nearby (D ∼ 0.8 Mpc) extremely metal-poor (Z ∼ 5% Z ) galaxy Leo A using Hubble Space Telescope ultraviolet (UV), optical, and near-infrared (NIR) imaging along with Keck/Low-Resolution Imaging Spectrograph and MMT/Binospec optical spectroscopy for 18 main-sequence OB stars…

2022 The Astrophysical Journal
eHST 13