Search Publications

COS-burst: Observations of the Impact of Starburst-driven Winds on the Properties of the Circum-galactic Medium
DOI: 10.3847/1538-4357/aa80dc Bibcode: 2017ApJ...846..151H

Heckman, Timothy; Wild, Vivienne; Borthakur, Sanchayeeta +2 more

We report on observations made with the Cosmic Origins Spectrograph (COS) on the Hubble Space Telescope (HST) using background quasi-stellar objects to probe the circum-galactic medium (CGM) around 17 low-redshift galaxies that are undergoing or have recently undergone a strong starburst (the COS-Burst program). The sightlines extend out to roughl…

2017 The Astrophysical Journal
eHST 80
Does a Differentiated, Carbonate-rich, Rocky Object Pollute the White Dwarf SDSS J104341.53+085558.2?
DOI: 10.3847/1538-4357/834/1/1 Bibcode: 2017ApJ...834....1M

Dufour, P.; Melis, Carl

We present spectroscopic observations of the dust- and gas-enshrouded, polluted, single white dwarf star SDSS J104341.53+085558.2 (hereafter SDSS J1043+0855). Hubble Space Telescope Cosmic Origins Spectrograph far-ultraviolet spectra combined with deep Keck HIRES optical spectroscopy reveal the elements C, O, Mg, Al, Si, P, S, Ca, Fe, and Ni and e…

2017 The Astrophysical Journal
eHST 79
Microlensing of Extremely Magnified Stars near Caustics of Galaxy Clusters
DOI: 10.3847/1538-4357/aa9575 Bibcode: 2017ApJ...850...49V

Miralda-Escudé, Jordi; Dai, Liang; Venumadhav, Tejaswi

Recent observations of lensed galaxies at cosmological distances have detected individual stars that are extremely magnified when crossing the caustics of lensing clusters. In idealized cluster lenses with smooth mass distributions, two images of a star of radius R approaching a caustic brighten as {t}-1/2 and reach a peak magnification…

2017 The Astrophysical Journal
eHST 79
Lensing Constraints on the Mass Profile Shape and the Splashback Radius of Galaxy Clusters
DOI: 10.3847/1538-4357/aa5c90 Bibcode: 2017ApJ...836..231U

Umetsu, Keiichi; Diemer, Benedikt

The lensing signal around galaxy clusters can, in principle, be used to test detailed predictions for their average mass profile from numerical simulations. However, the intrinsic shape of the profiles can be smeared out when a sample that spans a wide range of cluster masses is averaged in physical length units. This effect especially conceals ra…

2017 The Astrophysical Journal
eHST 79
The Dragonfly Nearby Galaxies Survey. III. The Luminosity Function of the M101 Group
DOI: 10.3847/1538-4357/aa615b Bibcode: 2017ApJ...837..136D

van Dokkum, Pieter; Abraham, Roberto; Danieli, Shany +4 more

We obtained follow-up HST observations of the seven low surface brightness galaxies discovered with the Dragonfly Telephoto Array in the field of the massive spiral galaxy M101. Out of the seven galaxies, only three were resolved into stars and are potentially associated with the M101 group at D = 7 Mpc. Based on HST ACS photometry in the broad F6…

2017 The Astrophysical Journal
eHST 79
Relations between the Sizes of Galaxies and Their Dark Matter Halos at Redshifts 0 < z < 3
DOI: 10.3847/1538-4357/aa62a6 Bibcode: 2017ApJ...838....6H

Pérez-González, Pablo G.; Ferguson, Henry C.; van der Wel, Arjen +6 more

We derive relations between the effective radii R eff of galaxies and the virial radii R 200c of their dark matter halos over the redshift range 0 < z < 3. For galaxies, we use the measured sizes from deep images taken with Hubble Space Telescope for the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey; f…

2017 The Astrophysical Journal
eHST 79
Connection between Stellar Mass Distributions within Galaxies and Quenching Since z = 2
DOI: 10.3847/1538-4357/aa5f14 Bibcode: 2017ApJ...837....2M

Tacchella, Sandro; Renzini, Alvio; Onodera, Masato +5 more

We study the history from z∼ 2 to z∼ 0 of the stellar mass assembly of quiescent and star-forming galaxies in a spatially resolved fashion. For this purpose, we use multi-wavelength imaging data from the Hubble Space Telescope (HST) over the GOODS fields and the Sloan Digital Sky Survey (SDSS) for the local population. We present the radial stella…

2017 The Astrophysical Journal
eHST 78
Gemini Near Infrared Field Spectrograph Observations of the Seyfert 2 Galaxy Mrk 573: In Situ Acceleration of Ionized and Molecular Gas off Fueling Flows
DOI: 10.3847/1538-4357/834/1/30 Bibcode: 2017ApJ...834...30F

Kraemer, S. B.; Crenshaw, D. M.; Storchi-Bergmann, T. +9 more

We present near-infrared and optical emission-line and stellar kinematics of the Seyfert 2 galaxy Mrk 573 using the Near-Infrared Field Spectrograph (NIFS) at Gemini North and Dual Imaging Spectrograph at Apache Point Observatory, respectively. By obtaining full kinematic maps of the infrared ionized and molecular gas and stellar kinematics in a ∼…

2017 The Astrophysical Journal
eHST 77
Survey of Cold Water Lines in Protoplanetary Disks: Indications of Systematic Volatile Depletion
DOI: 10.3847/1538-4357/aa70ee Bibcode: 2017ApJ...842...98D

van Dishoeck, Ewine F.; Fedele, Davide; Lis, Dariusz C. +11 more

We performed very deep searches for 2 ground-state water transitions in 13 protoplanetary disks with the HIFI instrument on board the Herschel Space Observatory, with integration times up to 12 hr per line. We also searched for, with shallower integrations, two other water transitions that sample warmer gas. The detection rate is low, and the uppe…

2017 The Astrophysical Journal
Herschel 77
Spectral Changes in the Hyperluminous Pulsar in NGC 5907 as a Function of Super-orbital Phase
DOI: 10.3847/1538-4357/834/1/77 Bibcode: 2017ApJ...834...77F

Harrison, F. A.; Stern, D.; Bachetti, M. +5 more

We present broadband, multi-epoch X-ray spectroscopy of the pulsating ultra-luminous X-ray source (ULX) in NGC 5907. Simultaneous XMM-Newton and NuSTAR data from 2014 are best described by a multicolor blackbody model with a temperature gradient as a function of accretion disk radius significantly flatter than expected for a standard thin accretio…

2017 The Astrophysical Journal
XMM-Newton 77