Search Publications

The Accretion History of EX Lup: A Century of Bursts, Outbursts, and Quiescence
DOI: 10.3847/1538-4357/acf2f4 Bibcode: 2023ApJ...957..113W

Fang, Min; Herczeg, Gregory J.; Johnstone, Doug +11 more

EX Lup is the archetype for the class of young stars that undergoes repeated accretion outbursts of ~5 mag at optical wavelengths that last for months. Despite extensive monitoring that dates back 130 yr, the accretion history of EX Lup remains mostly qualitative and has large uncertainties. We assess historical accretion rates of EX Lup by applyi…

2023 The Astrophysical Journal
Gaia 11
Standardized Luminosity of the Tip of the Red Giant Branch Utilizing Multiple Fields in NGC 4258 and the CATs Algorithm
DOI: 10.3847/1538-4357/acf4fb Bibcode: 2023ApJ...956...32L

Casertano, Stefano; Li, Siyang; Riess, Adam G. +6 more

The tip of the red giant branch provides a luminous standard candle for calibrating distance ladders that reach Type Ia supernova (SN Ia) hosts. However, recent work reveals that tip measurements vary at the ~0.1 mag level for different stellar populations and locations within a host, which may lead to inconsistencies along the distance ladder. We…

2023 The Astrophysical Journal
eHST 11
Hubble Space Telescope and Hyper-Suprime-Cam Weak-lensing Study of the Equal-mass Dissociative Merger CIZA J0107.7+5408
DOI: 10.3847/1538-4357/ac9fd3 Bibcode: 2023ApJ...942...23F

Clarke, Tracy E.; Giacintucci, Simona; Jee, M. James +6 more

A dissociative merger is formed by the interplay of ram pressure and gravitational forces, which can lead to a spatial displacement of the dark matter and baryonic components of the recently collided subclusters. CIZA J0107.7+5408 is a nearby (z = 0.105) dissociative merger that hosts two X-ray brightness peaks and a bimodal galaxy distribution. A…

2023 The Astrophysical Journal
eHST 11
Estimates of Proton and Electron Heating Rates Extended to the Near-Sun Environment
DOI: 10.3847/2041-8213/acf85e Bibcode: 2023ApJ...955L..28B

McComas, D. J.; Bale, S. D.; Cranmer, S. R. +11 more

A central problem of space plasma physics is how protons and electrons are heated in a turbulent, magnetized plasma. The differential heating of charged species due to dissipation of turbulent fluctuations plays a key role in solar wind evolution. Measurements from previous heliophysics missions have provided estimates of proton and electron heati…

2023 The Astrophysical Journal
Ulysses 11
Demographics of Protoplanetary Disks: A Simulated Population of Edge-on Systems
DOI: 10.3847/1538-4357/acbb01 Bibcode: 2023ApJ...945..130A

Perrin, Marshall D.; Ménard, François; Angelo, Isabel +9 more

The structure of protoplanetary disks plays an essential role in planet formation. A disk that is highly inclined, or "edge-on," is of particular interest since its geometry provides a unique opportunity to study the disk's vertical structure and radial extent. Candidate edge-on protoplanetary disks are typically identified via their unique spectr…

2023 The Astrophysical Journal
AKARI 11
SN 2023emq: A Flash-ionized Ibn Supernova with Possible C III Emission
DOI: 10.3847/2041-8213/ad103d Bibcode: 2023ApJ...959L..10P

Gromadzki, M.; Galbany, L.; Inserra, C. +16 more

SN 2023emq is a fast-evolving transient initially classified as a rare Type Icn supernova (SN), interacting with a H- and He-free circumstellar medium (CSM) around maximum light. Subsequent spectroscopy revealed the unambiguous emergence of narrow He lines, confidently placing SN 2023emq in the more common Type Ibn class. Photometrically, SN 2023e…

2023 The Astrophysical Journal
Gaia 11
Measuring the 8621 A Diffuse Interstellar Band in Gaia DR3 RVS Spectra: Obtaining a Clean Catalog by Marginalizing over Stellar Types
DOI: 10.3847/1538-4357/acd454 Bibcode: 2023ApJ...954..141S

Peek, J. E. G.; Zucker, Catherine; Finkbeiner, Douglas P. +2 more

Diffuse interstellar bands (DIBs) are broad absorption features associated with interstellar dust and can serve as chemical and kinematic tracers. Conventional measurements of DIBs in stellar spectra are complicated by residuals between observations and best-fit stellar models. To overcome this, we simultaneously model the spectrum as a combinatio…

2023 The Astrophysical Journal
Gaia 11
RR Lyrae Mid-infrared Period-Luminosity-Metallicity and Period-Wesenheit-Metallicity Relations Based on Gaia DR3 Parallaxes
DOI: 10.3847/1538-4357/acb20a Bibcode: 2023ApJ...945...83M

D'Orazi, Valentina; Dall'Ora, Massimo; Bono, Giuseppe +8 more

We present new empirical infrared period-luminosity-metallicity (PLZ) and period-Wesenheit-metallicity (PWZ) relations for RR Lyae based on the latest Gaia Early Data Release 3 (EDR3) parallaxes. The relations are provided in the Wide-field Infrared Survey Explorer (WISE) W1 and W2 bands, as well as in the W(W1, V - W1) and W(W2, V - W2) Wesenheit…

2023 The Astrophysical Journal
Gaia 11
Evidence for Population-dependent Vertical Motions and the Long-lived Nonsteady Lopsided Milky Way Warp
DOI: 10.3847/1538-4357/acab5b Bibcode: 2023ApJ...943...88L

Li, Xiang; Ting, Yuan-Sen; Wang, Hai-Feng +3 more

We present a Galactic disk vertical velocity analysis using OB type stars (OB stars), red clump (RC) stars, and main-sequence turnoff (MSTO) stars with different average age populations crossmatched with LAMOST DR5 and Gaia DR3. We show that the vertical velocities of the three populations clearly vary with the Galactocentric distance (R) and the …

2023 The Astrophysical Journal
Gaia 11
Orbital Decay in an Accreting and Eclipsing 13.7 Minute Orbital Period Binary with a Luminous Donor
DOI: 10.3847/2041-8213/ace7cf Bibcode: 2023ApJ...953L...1B

Kulkarni, S. R.; Riddle, Reed; Chakrabarty, Deepto +24 more

We report the discovery of ZTF J0127+5258, a compact mass-transferring binary with an orbital period of 13.7 minutes. The system contains a white dwarf accretor, which likely originated as a post-common envelope carbon-oxygen (CO) white dwarf, and a warm donor (T eff,donor = 16,400 ± 1000 K). The donor probably formed during a common en…

2023 The Astrophysical Journal
Gaia 11