Search Publications

Changing-look Event in NGC 3516: Continuum or Obscuration Variability?
DOI: 10.3847/1538-4357/ac42ca Bibcode: 2022ApJ...925...84M

Brenneman, Laura W.; Kriss, Gerard A.; Mehdipour, Missagh +6 more

The Seyfert-1 galaxy NGC 3516 has undergone major spectral changes in recent years. In 2017 we obtained Chandra, NuSTAR, and Swift observations during its new low-flux state. Using these observations, we model the spectral energy distribution (SED) and the intrinsic X-ray absorption, and compare the results with those from historical observations …

2022 The Astrophysical Journal
XMM-Newton 25
The Physical Properties of the SVS 13 Protobinary System: Two Circumstellar Disks and a Spiraling Circumbinary Disk in the Making
DOI: 10.3847/1538-4357/ac3b50 Bibcode: 2022ApJ...930...91D

Ho, Paul T. P.; Zapata, Luis A.; Carrasco-González, Carlos +13 more

We present Very Large Array (VLA) and Atacama Large Millimeter/submillimeter Array (ALMA) observations of the close (0.″3 = 90 au separation) protobinary system SVS 13. We detect two small circumstellar disks (radii ~12 and ~9 au in dust, and ~30 au in gas) with masses of ~0.004-0.009 M for VLA 4A (the western component) and ~0.009-0.…

2022 The Astrophysical Journal
Gaia 25
Disentangling the formation mechanisms of nuclear star clusters
DOI: 10.1051/0004-6361/202039778 Bibcode: 2022A&A...658A.172F

Fahrion, Katja; Leaman, Ryan; van de Ven, Glenn +1 more

Nuclear star clusters (NSCs) are massive star clusters found ubiquitously in the centres of galaxies, from the dwarf regime to massive ellipticals and spirals. The fraction of nucleated galaxies is as high as > 90% at Mgal ∼ 109 M. However, how NSC formation mechanisms work in different regimes and what determi…

2022 Astronomy and Astrophysics
eHST 25
Early Results from GLASS-JWST. VI. Extreme Rest-optical Equivalent Widths Detected in NIRISS Wide Field Slitless Spectroscopy
DOI: 10.3847/2041-8213/ac9f17 Bibcode: 2022ApJ...940L..52B

Vulcani, B.; Brammer, G.; Treu, T. +27 more

Wide Field Slitless Spectroscopy (WFSS) provides a powerful tool for detecting strong line emission in star-forming galaxies (SFGs) without the need for target preselection. As part of the GLASS-JWST Early Release Science (ERS) program, we leverage the near-infrared wavelength capabilities of NIRISS (1-2.2 µm) to observe rest-optical emissio…

2022 The Astrophysical Journal
JWST 25
Nothing to see here: failed supernovae are faint or rare
DOI: 10.1093/mnras/stac1308 Bibcode: 2022MNRAS.514.1188B

Fraser, M.; Byrne, R. A.

The absence of Type IIP core-collapse supernovae arising from progenitors above 17 solar masses suggests the existence of another evolutionary path by which massive stars end their lives. The direct collapse of a stellar core to a black hole without the production of a bright, explosive transient is expected to produce a long-lived, dim, red trans…

2022 Monthly Notices of the Royal Astronomical Society
eHST 25
Gaia DR3 in 6D: the search for fast hypervelocity stars and constraints on the galactic centre environment
DOI: 10.1093/mnras/stac1777 Bibcode: 2022MNRAS.515..767M

Marchetti, Tommaso; Evans, Fraser A.; Rossi, Elena Maria

The third data release (DR3) of the European Space Agency satellite Gaia provides coordinates, parallaxes, proper motions, and radial velocities for a sample of ~34 million stars. We use the combined 6D phase space information to search for hypervelocity stars (HVSs), unbound stars accelerated by dynamical processes happening in the Galactic Centr…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 25
New Constraints on the Spin of the Black Hole Cygnus X-1 and the Physical Properties of its Accretion Disk Corona
DOI: 10.3847/1538-4357/ac7725 Bibcode: 2022ApJ...934....4K

Krawczynski, H.; Beheshtipour, B.

We present a new analysis of NuSTAR and Suzaku observations of the black hole Cygnus X-1 in the intermediate state. The analysis is performed using kerrC, a new model for analyzing spectral and spectropolarimetric X-ray observations of black holes. kerrC builds on a large library of simulated black holes in X-ray binaries. The model accounts for t…

2022 The Astrophysical Journal
Suzaku 25
Angular clustering properties of the DESI QSO target selection using DR9 Legacy Imaging Surveys
DOI: 10.1093/mnras/stab3252 Bibcode: 2022MNRAS.509.3904C

Myers, Adam D.; Palanque-Delabrouille, Nathalie; Yèche, Christophe +12 more

The quasar target selection for the upcoming survey of the Dark Energy Spectroscopic Instrument (DESI) will be fixed for the next 5 yr. The aim of this work is to validate the quasar selection by studying the impact of imaging systematics as well as stellar and galactic contaminants, and to develop a procedure to mitigate them. Density fluctuation…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 25
Direct First Parker Solar Probe Observation of the Interaction of Two Successive Interplanetary Coronal Mass Ejections in 2020 November
DOI: 10.3847/1538-4357/ac590b Bibcode: 2022ApJ...930...88N

Reeves, Katharine K.; Hess, Phillip; Nieves-Chinchilla, Teresa +20 more

We investigate the effects of the evolutionary processes in the internal magnetic structure of two interplanetary coronal mass ejections (ICMEs) detected in situ between 2020 November 29 and December 1 by the Parker Solar Probe (PSP). The sources of the ICMEs were observed remotely at the Sun in EUV and subsequently tracked to their coronal counte…

2022 The Astrophysical Journal
SOHO 25
Photometric Observations of the Binary Near-Earth Asteroid (65803) Didymos in 2015-2021 Prior to DART Impact
DOI: 10.3847/PSJ/ac7be1 Bibcode: 2022PSJ.....3..175P

Carry, B.; Souami, D.; Dotto, E. +24 more

We performed photometric observations of the binary near-Earth asteroid (65803) Didymos in support of the Double Asteroid Redirection Test (DART) mission that will test the Kinetic Impactor technology for diverting dangerous asteroids. It will hit the Didymos secondary, called Dimorphos, on 2022 September 26. We observed Didymos with 11 telescopes…

2022 The Planetary Science Journal
Gaia 25