Search Publications

Herschel Gould Belt Survey Observations of Dense Cores in the Cepheus Flare Clouds
DOI: 10.3847/1538-4357/abc016 Bibcode: 2020ApJ...904..172D

Ward-Thompson, Derek; Arzoumanian, Doris; Di Francesco, James +17 more

We present Herschel SPIRE and PACS maps of the Cepheus Flare clouds L1157, L1172, L1228, L1241, and L1251, observed by the Herschel Gould Belt Survey of nearby star-forming molecular clouds. Through modified blackbody fits to the SPIRE and PACS data, we determine typical cloud column densities of (0.5-1.0) × 1021 cm-2 and typ…

2020 The Astrophysical Journal
Herschel 25
The White Dwarf Binary Pathways Survey. V. The Gaia White Dwarf Plus AFGK Binary Sample and the Identification of 23 Close Binaries
DOI: 10.3847/1538-4357/abc017 Bibcode: 2020ApJ...905...38R

Gänsicke, B. T.; Rebassa-Mansergas, A.; Raddi, R. +22 more

Close white dwarf binaries consisting of a white dwarf and an A-, F-, G-, or K-type main-sequence star, henceforth close WD+AFGK binaries, are ideal systems to understand the nature of type Ia supernovae progenitors and to test binary evolution models. In this work we identify 775 WD+AFGK candidates from TGAS (The Tycho-Gaia Astrometric Solution) …

2020 The Astrophysical Journal
Gaia 25
Discovery of a Remarkably Powerful Broad Absorption-line Quasar Outflow in SDSS J135246.37+423923.5
DOI: 10.3847/1538-4357/ab6f72 Bibcode: 2020ApJ...891...53C

Gallagher, Sarah C.; Terndrup, Donald M.; Leighly, Karen M. +2 more

Broad absorption-line (BAL) features in quasar spectra reveal an unambiguous signature of energetic outflows from central supermassive black holes, and thus, BAL quasars are prime targets for investigating the potential process of luminous quasar feedback on galaxies. We analyzed the rest-UV spectrum of an "overlapping trough" iron low-ionization …

2020 The Astrophysical Journal
Herschel eHST 25
The Formation Height of Millimeter-wavelength Emission in the Solar Chromosphere
DOI: 10.3847/2041-8213/ab75ac Bibcode: 2020ApJ...891L...8M

Martínez-Sykora, Juan; De Pontieu, Bart; Chintzoglou, Georgios +1 more

In the past few years, the ALMA radio telescope has become available for solar observations. ALMA diagnostics of the solar atmosphere are of high interest because of the theoretically expected linear relationship between the brightness temperature at millimeter wavelengths and the local gas temperature in the solar atmosphere. Key for the interpre…

2020 The Astrophysical Journal
IRIS 25
The PIPER Survey. I. An Initial Look at the Intergalactic Globular Cluster Population in the Perseus Cluster
DOI: 10.3847/1538-4357/ab6992 Bibcode: 2020ApJ...890..105H

Wittmann, Carolin; Lisker, Thorsten; Romanowsky, Aaron J. +7 more

We describe the goals and first results of the Program for Imaging of the PERseus cluster of galaxies (PIPER). The first phase of the program builds on imaging of fields obtained with the Hubble Space Telescope (HST) Advanced Camera for Surveys (ACS)/WFC and WFC3/UVIS cameras. Our PIPER target fields with HST include major early-type galaxies incl…

2020 The Astrophysical Journal
eHST 25
WISEA J083011.95+283716.0: A Missing Link Planetary-mass Object
DOI: 10.3847/1538-4357/ab8d25 Bibcode: 2020ApJ...895..145B

Wisniewski, John; Kirkpatrick, J. Davy; Burgasser, Adam J. +17 more

We present the discovery of WISEA J083011.95+283716.0, the first Y-dwarf candidate identified through the "Backyard Worlds: Planet 9" citizen science project. We identified this object as a red, fast-moving source with a faint W2 detection in multiepoch AllWISE and unWISE images. We have characterized this object with Spitzer and Hubble Space Tele…

2020 The Astrophysical Journal
eHST 25
ALMA CO Observations of Gamma-Ray Supernova Remnant N132D in the Large Magellanic Cloud: Possible Evidence for Shocked Molecular Clouds Illuminated by Cosmic-Ray Protons
DOI: 10.3847/1538-4357/abb469 Bibcode: 2020ApJ...902...53S

Filipović, M. D.; Vink, J.; Rowell, G. +23 more

N132D is the brightest gamma-ray supernova remnant (SNR) in the Large Magellanic Cloud (LMC). We carried out 12CO(J = 1-0, 3-2) observations toward the SNR using the Atacama Large Millimeter/submillimeter Array (ALMA) and Atacama Submillimeter Telescope Experiment. We find diffuse CO emission not only at the southern edge of the SNR as …

2020 The Astrophysical Journal
eHST 25
SCExAO/CHARIS High-contrast Imaging of Spirals and Darkening Features in the HD 34700 A Protoplanetary Disk
DOI: 10.3847/1538-4357/aba8f6 Bibcode: 2020ApJ...900..135U

Currie, Thayne; Kwon, Jungmi; Tamura, Motohide +27 more

We present Subaru/SCExAO+Coronagraphic High Angular Resolution Imaging Spectrograph (CHARIS) broadband (JHK-band) integral field spectroscopy of HD 34700 A. CHARIS data recover HD 34700 A's disk ring and confirm multiple spirals discovered by Monnier et al. We set limits on substellar companions of ∼12 MJup at 0"3 (in the ring gap) and …

2020 The Astrophysical Journal
Gaia 24
Supernova Interaction with a Dense Detached Shell in SN 2001em
DOI: 10.3847/1538-4357/abb460 Bibcode: 2020ApJ...902...55C

Chandra, Poonam; Fransson, Claes; Chevalier, Roger A. +2 more

We carry out a comprehensive analysis of supernova SN 2001em covering a period of 19 yr since discovery. SN 2001em is the oldest supernova known to have undergone a metamorphosis from a stripped envelope to an interacting supernova. An early spectrum indicates it exploded as a Type Ib supernova. Later, the ejecta caught up with a dense circumstell…

2020 The Astrophysical Journal
XMM-Newton 24
PSR J1641+3627F: A Low-mass He White Dwarf Orbiting a Possible High-mass Neutron Star in the Globular Cluster M13
DOI: 10.3847/1538-4357/abc345 Bibcode: 2020ApJ...905...63C

Cadelano, Mario; Pallanca, Cristina; Salaris, Maurizio +5 more

We report on the discovery of the companion star to the millisecond pulsar J1631+3627F in the globular cluster M13. By means of a combination of optical and near-UV high-resolution observations obtained with the Hubble Space Telescope, we identified the counterpart at the radio source position. Its location in the color-magnitude diagrams reveals …

2020 The Astrophysical Journal
Gaia eHST 24