Search Publications

The “UV-route” to Search for Blue Straggler Stars in Globular Clusters: First Results from the HST UV Legacy Survey
DOI: 10.3847/1538-4357/aa6891 Bibcode: 2017ApJ...839...64R

Dalessandro, E.; Nardiello, D.; Vesperini, E. +4 more

We used data from the Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters to select the Blue Straggler Star (BSS) population in four intermediate/high density systems (namely NGC 2808, NGC 6388, NGC 6541, and NGC 7078) through a “UV-guided search.” This procedure consists of using the F275W images in each cluster to construct the…

2017 The Astrophysical Journal
eHST 34
Importance of CME Radial Expansion on the Ability of Slow CMEs to Drive Shocks
DOI: 10.3847/1538-4357/aa8ef9 Bibcode: 2017ApJ...848...75L

Lugaz, Noé; Farrugia, Charles J.; Winslow, Reka M. +3 more

Coronal mass ejections (CMEs) may disturb the solar wind by overtaking it or expanding into it, or both. CMEs whose front moves faster in the solar wind frame than the fast magnetosonic speed drive shocks. Such shocks are important contributors to space weather, by triggering substorms, compressing the magnetosphere, and accelerating particles. In…

2017 The Astrophysical Journal
SOHO 34
Exploring the Inner Acceleration Region of Solar Wind: A Study Based on Coronagraphic UV and Visible Light Data
DOI: 10.3847/1538-4357/aa7de4 Bibcode: 2017ApJ...846...86B

Bemporad, A.

This work combined coronagraphic visible light (VL) and UV data to provide with an unprecedented view of the inner corona where the nascent solar wind is accelerated. The UV (H I Lyα) and VL (polarized brightness) images (reconstructed with SOHO/UVCS, LASCO, and Mauna Loa data) have been analyzed with the Doppler dimming technique to provide for t…

2017 The Astrophysical Journal
SOHO 34
Specific Frequencies and Luminosity Profiles of Cluster Galaxies and Intracluster Light in Abell 1689
DOI: 10.3847/1538-4357/aa8f44 Bibcode: 2017ApJ...849....6A

Blakeslee, J. P.; Alamo-Martínez, K. A.

We present magnitudes and profile fits for 180 galaxies in the central field of the massive lensing cluster Abell 1689 using very deep imaging with the Hubble Space Telescope Advanced Camera for Surveys in the F814W bandpass. Previous work revealed an exceptionally large number of globular clusters (GCs) in A1689 and mapped their number density di…

2017 The Astrophysical Journal
eHST 34
Photometric Determination of the Mass Accretion Rates of Pre-main-sequence Stars. V. Recent Star Formation in the 30 Dor Nebula
DOI: 10.3847/1538-4357/aa85e9 Bibcode: 2017ApJ...846..110D

Panagia, Nino; Beccari, Giacomo; De Marchi, Guido

We report on the properties of the low-mass stars that recently formed in the central ∼ 2\buildrel{ \prime}\over{.} 7× 2\buildrel{ \prime}\over{.} 7 of 30 Dor, including the R136 cluster. Using the photometric catalog of De Marchi et al., based on observations with the Hubble Space Telescope, and the most recent extinction law for this field, we i…

2017 The Astrophysical Journal
eHST 34
Shedding Light on the Compton-thick Active Galactic Nucleus in the Ultraluminous Infrared Galaxy UGC 5101 with Broadband X-Ray Spectroscopy
DOI: 10.3847/1538-4357/835/2/179 Bibcode: 2017ApJ...835..179O

Imanishi, Masatoshi; Tanimoto, Atsushi; Ueda, Yoshihiro +3 more

We report the broadband X-ray spectra of the ultraluminous infrared galaxy (ULIRG) UGC 5101 in the 0.25-100 keV band observed with the Swift/Burst Alert Telescope (BAT), Nuclear Spectroscopic Telescope Array (NuSTAR), Suzaku, XMM-Newton, and Chandra. A Compton-thick active galactic nucleus (AGN) obscured with a hydrogen column density of ≈ 1.3× {1…

2017 The Astrophysical Journal
Suzaku XMM-Newton 34
Lyα and UV Sizes of Green Pea Galaxies
DOI: 10.3847/1538-4357/aa6337 Bibcode: 2017ApJ...838....4Y

Leitherer, Claus; Wofford, Aida; Malhotra, Sangeeta +4 more

Green Peas are nearby analogs of high-redshift Lyα-emitting galaxies (LAEs). To probe their Lyα escape, we study the spatial profiles of Lyα and UV continuum emission of 24 Green Pea galaxies using the Cosmic Origins Spectrograph (COS) on the Hubble Space Telescope. We extract the spatial profiles of Lyα emission from their 2D COS spectra, and of …

2017 The Astrophysical Journal
eHST 34
The Rotation-Activity Correlations in K and M Dwarfs. II. New Constraints on the Dynamo Mechanisms in Late-K and M Dwarfs Before and At the Transition to Complete Convection
DOI: 10.3847/1538-4357/aa5cad Bibcode: 2017ApJ...837...96H

Mullan, D. J.; Gebran, M.; Houdebine, E. R. +2 more

We study the rotation-activity correlations (RACs) in a sample of stars from spectral type dK4 to dM4. We study RACs using chromospheric data and coronal data. We study the Ca II line surface fluxes-P/\sin I RACs. We fit the RACs with linear homoscedastic and heteroscedastic regression models. We find that these RACs differ substantially from one …

2017 The Astrophysical Journal
Hipparcos 34
A Hubble Space Telescope Survey for Novae in M87. II. Snuffing out the Maximum Magnitude-Rate of Decline Relation for Novae as a Non-standard Candle, and a Prediction of the Existence of Ultrafast Novae
DOI: 10.3847/1538-4357/aa65cd Bibcode: 2017ApJ...839..109S

Welch, D. L.; Lauer, Tod R.; Mikołajewska, Joanna +9 more

The extensive grid of numerical simulations of nova eruptions from the work of Yaron et al. first predicted that some classical novae might significantly deviate from the Maximum Magnitude-Rate of Decline (MMRD) relation, which purports to characterize novae as standard candles. Kasliwal et al. have announced the observational detection of a new c…

2017 The Astrophysical Journal
eHST 34
Investigating the Origins of Two Extreme Solar Particle Events: Proton Source Profile and Associated Electromagnetic Emissions
DOI: 10.3847/1538-4357/aa6a13 Bibcode: 2017ApJ...839...79K

Vainio, Rami; Valtonen, Eino; Pohjolainen, Silja +13 more

We analyze the high-energy particle emission from the Sun in two extreme solar particle events in which protons are accelerated to relativistic energies and can cause a significant signal even in the ground-based particle detectors. Analysis of a relativistic proton event is based on modeling of the particle transport and interaction, from a near-…

2017 The Astrophysical Journal
SOHO 34