Search Publications

Absolute Calibration of Cepheid Period-Luminosity Relations in NGC 4258
DOI: 10.3847/1538-4357/ac51db Bibcode: 2022ApJ...940...64Y

Casertano, Stefano; Filippenko, Alexei V.; Riess, Adam G. +6 more

Owing to its accurate distance measured from water-maser motions, NGC 4258 is one of the most important anchors for calibrating the Cepheid period-luminosity relations (PLRs). We expand on previous efforts and carry out a new Cepheid search in this system using the Hubble Space Telescope. We discover and measure a sample of 669 Cepheids in four ne…

2022 The Astrophysical Journal
Gaia eHST 19
Multi-spacecraft Observations of the Evolution of Interplanetary Coronal Mass Ejections between 0.3 and 2.2 au: Conjunctions with the Juno Spacecraft
DOI: 10.3847/1538-4357/ac731a Bibcode: 2022ApJ...933..127D

Lugaz, Noé; Scolini, Camilla; Winslow, Réka M. +4 more

We present a catalog of 35 interplanetary coronal mass ejections (ICMEs) observed by the Juno spacecraft and at least one other spacecraft during its cruise phase to Jupiter. We identify events observed by MESSENGER, Venus Express, Wind, and STEREO with magnetic features that can be matched unambiguously with those observed by Juno. A multi-spacec…

2022 The Astrophysical Journal
Ulysses VenusExpress 19
Ensemble Simulations of the 2012 July 12 Coronal Mass Ejection with the Constant-turn Flux Rope Model
DOI: 10.3847/1538-4357/ac73f3 Bibcode: 2022ApJ...933..123S

Pogorelov, Nikolai V.; Arge, Charles N.; Singh, Talwinder +1 more

Flux-rope-based magnetohydrodynamic modeling of coronal mass ejections (CMEs) is a promising tool for prediction of the CME arrival time and magnetic field at Earth. In this work, we introduce a constant-turn flux rope model and use it to simulate the 2012 July 12 16:48 CME in the inner heliosphere. We constrain the initial parameters of this CME …

2022 The Astrophysical Journal
SOHO 19
HyGAL: Characterizing the Galactic Interstellar Medium with Observations of Hydrides and Other Small Molecules. I. Survey Description and a First Look Toward W3(OH), W3 IRS5, and NGC 7538 IRS1
DOI: 10.3847/1538-4357/ac5409 Bibcode: 2022ApJ...930..141J

Menten, K. M.; Falgarone, E.; Godard, B. +23 more

The HyGAL Stratospheric Observatory for Infrared Astronomy legacy program surveys six hydride molecules-ArH+, OH+, H2O+, SH, OH, and CH-and two atomic constituents-C+ and O-within the diffuse interstellar medium (ISM) by means of absorption-line spectroscopy toward 25 bright Galactic backgroun…

2022 The Astrophysical Journal
Herschel 19
Another Look at Erupting Minifilaments at the Base of Solar X-Ray Polar Coronal "Standard" and "Blowout" Jets
DOI: 10.3847/1538-4357/ac473f Bibcode: 2022ApJ...927..127S

Panesar, Navdeep K.; Moore, Ronald L.; Sterling, Alphonse C.

We examine 21 solar polar coronal jets that we identify in soft X-ray images obtained from the Hinode/X-ray telescope (XRT). We identify 11 of these as blowout jets and four as standard jets (with six uncertain), based on their X-ray-spire widths being respectively wide or narrow (compared to the jet's base) in the XRT images. From corresponding e…

2022 The Astrophysical Journal
Hinode 19
Magnetic Field Intermittency in the Solar Wind: Parker Solar Probe and SolO Observations Ranging from the Alfvén Region up to 1 AU
DOI: 10.3847/1538-4357/ac7aa2 Bibcode: 2022ApJ...934..143S

Fedorov, A.; Louarn, P.; Velli, Marco +19 more

Parker Solar Probe (PSP) and SolO data are utilized to investigate magnetic field intermittency in the solar wind (SW). Small-scale intermittency (20-100 d i ) is observed to radially strengthen when methods relying on higher-order moments are considered (SF q ; SDK), but no clear trend is observed at larger scales. However,…

2022 The Astrophysical Journal
SolarOrbiter 19
Supernova Remnants in M83 as Observed with MUSE
DOI: 10.3847/1538-4357/ac5aa3 Bibcode: 2022ApJ...929..144L

Della Bruna, Lorenza; Blair, William P.; Adamo, Angela +4 more

Here we describe a new study of the supernova remnants (SNRs) and SNR candidates in nearby face-on spiral galaxy M83, based primarily on MUSE integral field spectroscopy. Our revised catalog of SNR candidates in M83 has 366 objects, 81 of which are reported here for the first time. Of these, 229 lie within the MUSE observation region, 160 of which…

2022 The Astrophysical Journal
eHST 19
The Candidate Progenitor Companion Star of the Type Ib/c SN 2013ge
DOI: 10.3847/2041-8213/ac5890 Bibcode: 2022ApJ...929L..15F

Van Dyk, Schuyler D.; Filippenko, Alexei V.; Williams, Benjamin F. +17 more

This Letter presents the detection of a source at the position of the Type Ib/c supernova (SN) 2013ge more than four years after the radioactive component is expected to have faded. This source could mark the first post-SN direct detection of a surviving companion to a stripped-envelope Type Ib/c explosion. We test this hypothesis and find the sha…

2022 The Astrophysical Journal
eHST 19
Magellan/IMACS Spectroscopy of Grus I: A Low Metallicity Ultra-faint Dwarf Galaxy
DOI: 10.3847/1538-4357/ac96ed Bibcode: 2022ApJ...939...41C

Li, Ting S.; Frebel, Anna; Simon, Joshua D. +3 more

We present a chemodynamical study of the Grus I ultra-faint dwarf galaxy (UFD) from medium-resolution (R ~ 11,000) Magellan/IMACS spectra of its individual member stars. We identify eight confirmed members of Grus I, based on their low metallicities and coherent radial velocities, and four candidate members for which only velocities are derived. I…

2022 The Astrophysical Journal
Gaia 19
Evolution of X-Ray Activity in <25 Myr Old Pre-main Sequence Stars
DOI: 10.3847/1538-4357/ac7c69 Bibcode: 2022ApJ...935...43G

Garmire, Gordon P.; Feigelson, Eric D.; Broos, Patrick S. +4 more

Measuring the evolution of X-ray emission from pre-main-sequence (PMS) stars gives insight into two issues: the response of magnetic dynamo processes to changes in the interior structure, and the effects of high-energy radiation on protoplanetary disks and primordial planetary atmospheres. We present a sample of 6003 stars with ages 7-25 Myr in 10…

2022 The Astrophysical Journal
Gaia 19