Search Publications

Models of the Hydrodynamic Histories of Post-AGB Stars. I. Multiflow Shaping of OH 231.8+04.2
DOI: 10.3847/1538-4357/aa77f0 Bibcode: 2017ApJ...843..108B

Frank, Adam; Balick, Bruce; Liu, Baowei +1 more

We present a detailed hydrodynamic model that matches the present structure of the well-observed preplanetary nebula (“pPN”) OH 231.8+04.2 (“OH231”). The purpose of the model is to present a physically justified and coherent picture of its evolutionary history from about 100 years from the start of the formation of its complex outer structures to …

2017 The Astrophysical Journal
eHST 18
Variable Stars in Local Group Galaxies. III. And VII, NGC 147, and NGC 185: Insight into the Building Blocks of the M31 Halo
DOI: 10.3847/1538-4357/aa738d Bibcode: 2017ApJ...842...60M

Stetson, P. B.; Bono, G.; Fiorentino, G. +5 more

We present the discovery of 1568 RR Lyrae stars in three of the most luminous M31 satellites: And VII (573), NGC 147 (177), and NGC 185 (818). We use their properties to study the formation history of Local Group spiral haloes, and in particular, to infer about the nature of their possible building blocks by comparison with available data for RR L…

2017 The Astrophysical Journal
eHST 18
The Molecular Cloud S242: Physical Environment and Star-formation Activities
DOI: 10.3847/1538-4357/aa7da2 Bibcode: 2017ApJ...845...34D

Dewangan, L. K.; Ojha, D. K.; Janardhan, P. +3 more

We present a multi-wavelength study to probe the star-formation (SF) processes on a larger scale (∼ 1\buildrel{\circ}\over{.} 05× 0\buildrel{\circ}\over{.} 56) around the S242 site. The S242 molecular cloud is depicted in a velocity range from -3.25 to 4.55 km s-1 and has a spatially elongated appearance. Based on the virial analysis, t…

2017 The Astrophysical Journal
Herschel 18
ZFIRE: Similar Stellar Growth in Hα-emitting Cluster and Field Galaxies at z ~ 2
DOI: 10.3847/1538-4357/834/2/101 Bibcode: 2017ApJ...834..101T

Papovich, Casey; Kewley, Lisa J.; Kacprzak, Glenn G. +13 more

We compare galaxy scaling relations as a function of environment at z∼ 2 with our ZFIRE survey12 where we have measured Hα fluxes for 90 star-forming galaxies selected from a mass-limited ({log}({M}\star /{M})> 9) sample based on ZFOURGE.13 The cluster galaxies (37) are part of a confirmed system at…

2017 The Astrophysical Journal
eHST 17
A Catalog Sample of Low-mass Galaxies Observed in X-Rays with Central Candidate Black Holes
DOI: 10.3847/1538-4357/aa5f4f Bibcode: 2017ApJ...837...66N

Nucita, A. A.; De Paolis, F.; Ingrosso, G. +2 more

We present a sample of X-ray-selected candidate black holes in 51 low-mass galaxies with z ≤ 0.055 and masses up to 1010 M obtained by cross-correlating the NASA-SLOAN Atlas with the 3XMM catalog. We have also searched in the available catalogs for radio counterparts of the black hole candidates and find that 19 of the prev…

2017 The Astrophysical Journal
XMM-Newton 17
AGILE Observations of the Gravitational-wave Source GW170817: Constraining Gamma-Ray Emission from an NS-NS Coalescence
DOI: 10.3847/2041-8213/aa965d Bibcode: 2017ApJ...850L..27V

Antonelli, L. A.; Costa, E.; Barbiellini, G. +39 more

The LIGO-Virgo Collaboration (LVC) detected, on 2017 August 17, an exceptional gravitational-wave (GW) event temporally consistent within ∼ 1.7 {{s}} with the GRB 1708117A observed by Fermi-GBM and INTEGRAL. The event turns out to be compatible with a neutron star-neutron star (NS-NS) coalescence that subsequently produced a radio/optical/X-ray tr…

2017 The Astrophysical Journal
INTEGRAL 17
Discovery of a Very Bright and Intrinsically Very Luminous, Strongly Lensed Lyα Emitting Galaxy at z = 2.82 in the BOSS Emission-Line Lens Survey
DOI: 10.3847/2041-8213/834/2/L18 Bibcode: 2017ApJ...834L..18M

Brownstein, Joel R.; Marques-Chaves, Rui; Oguri, Masamune +9 more

We report the discovery of a very bright (r = 20.16), highly magnified, and yet intrinsically very luminous Lyα emitter (LAE) at z=2.82. This system comprises four images in the observer plane with a maximum separation of ∼ 6\prime\prime and it is lensed by a z=0.55 massive early-type galaxy. It was initially identified in the Baryon Os…

2017 The Astrophysical Journal
Gaia 17
Test of Weak Equivalence Principle with the Multi-band Timing of the Crab Pulsar
DOI: 10.3847/1538-4357/aa61fb Bibcode: 2017ApJ...837..134Z

Zhang, Yueyang; Gong, Biping

The Weak Equivalent Principle (WEP) can be tested through the parameterized post-Newtonian parameter γ, representing the space curvature produced by unit rest mass. The parameter γ in turn has been constrained by comparing the arrival times of photons originating in distant transient events, such as gamma-ray bursts, fast radio bursts, and giant p…

2017 The Astrophysical Journal
INTEGRAL 17
Evolution of Molecular Clouds in the Superwind Galaxy NGC 1808 Probed by ALMA Observations
DOI: 10.3847/1538-4357/aa91cb Bibcode: 2017ApJ...849...90S

Salak, Dragan; Tomiyasu, Yuto; Nakai, Naomasa +3 more

ALMA imaging of the cold molecular medium in the nearby starburst galaxy NGC 1808 is presented. The observations reveal the distribution of molecular gas, traced by 12CO (1-0) and 12CO (3-2), and continuum (93 and 350 GHz) across the central 1 kpc starburst region at a high resolution of ∼ 1\prime\prime . A molecul…

2017 The Astrophysical Journal
eHST 17
Herschel Spectroscopy of Early-type Galaxies
DOI: 10.3847/1538-4357/aa6d83 Bibcode: 2017ApJ...840...51L

Young, Lisa M.; Crocker, Alison; Lapham, Ryen Carl

We present Herschel spectroscopy of atomic lines arising in photodissociation regions as well as ionization regions of nearby early-type galaxies (ETGs), focusing on the volume-limited Atlas3D sample. Our data include the [C II], [O I], and [N II] 122 and 205 µm lines, along with ancillary data including CO and H I maps. We find that ETGs ha…

2017 The Astrophysical Journal
Herschel 17