Search Publications

Elongation of Flare Ribbons
DOI: 10.3847/1538-4357/aa6341 Bibcode: 2017ApJ...838...17Q

Qiu, Jiong; Longcope, Dana W.; Cassak, Paul A. +1 more

We present an analysis of the apparent elongation motion of flare ribbons along the polarity inversion line (PIL), as well as the shear of flare loops in several two-ribbon flares. Flare ribbons and loops spread along the PIL at a speed ranging from a few to a hundred km s-1. The shear measured from conjugate footpoints is consistent wi…

2017 The Astrophysical Journal
SOHO 54
Luminous and Variable Stars in M31 and M33. IV. Luminous Blue Variables, Candidate LBVs, B[e] Supergiants, and the Warm Hypergiants: How to Tell Them Apart
DOI: 10.3847/1538-4357/aa582e Bibcode: 2017ApJ...836...64H

Humphreys, Roberta M.; Gordon, Michael S.; Martin, John C. +2 more

In this series of papers we have presented the results of a spectroscopic survey of luminous stars in the nearby spirals M31 and M33. Here, we present spectroscopy of 132 additional stars. Most have emission-line spectra, including luminous blue variables (LBVs) and candidate LBVs, Fe II emission line stars, the B[e] supergiants, and the warm hype…

2017 The Astrophysical Journal
eHST 54
Absolute Ages and Distances of 22 GCs Using Monte Carlo Main-sequence Fitting
DOI: 10.3847/1538-4357/aa6574 Bibcode: 2017ApJ...838..162O

Chaboyer, Brian; O'Malley, Erin M.; Gilligan, Christina

The recent Gaia Data Release 1 of stellar parallaxes provides ample opportunity to find metal-poor main-sequence stars with precise parallaxes. We select 21 such stars with parallax uncertainties better than σ π /π ≤ 0.10 and accurate abundance determinations suitable for testing metal-poor stellar evolution models and determining the …

2017 The Astrophysical Journal
Gaia eHST 54
The Sirius System and Its Astrophysical Puzzles: Hubble Space Telescope and Ground-based Astrometry
DOI: 10.3847/1538-4357/aa6af8 Bibcode: 2017ApJ...840...70B

Schaefer, Gail H.; Bond, Howard E.; Burleigh, Matthew R. +11 more

Sirius, the seventh-nearest stellar system, is a visual binary containing the metallic-line A1 V star Sirius A, the brightest star in the sky, orbited in a 50.13 year period by Sirius B, the brightest and nearest white dwarf (WD). Using images obtained over nearly two decades with the Hubble Space Telescope (HST), along with photographic observati…

2017 The Astrophysical Journal
eHST 54
The PdBI Arcsecond Whirlpool Survey (PAWS): The Role of Spiral Arms in Cloud and Star Formation
DOI: 10.3847/1538-4357/836/1/62 Bibcode: 2017ApJ...836...62S

Leroy, Adam K.; Meidt, Sharon E.; Hughes, Annie +9 more

The process that leads to the formation of the bright star-forming sites observed along prominent spiral arms remains elusive. We present results of a multi-wavelength study of a spiral arm segment in the nearby grand-design spiral galaxy M51 that belongs to a spiral density wave and exhibits nine gas spurs. The combined observations of the (ioniz…

2017 The Astrophysical Journal
eHST 54
Evidence for a Time Lag in Solar Modulation of Galactic Cosmic Rays
DOI: 10.3847/2041-8213/aa9373 Bibcode: 2017ApJ...849L..32T

Tomassetti, Nicola; Orcinha, Miguel; Barão, Fernando +1 more

The solar modulation effect of cosmic rays in the heliosphere is an energy-, time-, and particle-dependent phenomenon that arises from a combination of basic particle transport processes such as diffusion, convection, adiabatic cooling, and drift motion. Making use of a large collection of time-resolved cosmic-ray data from recent space missions, …

2017 The Astrophysical Journal
SOHO 53
Mass-loss Rates from Coronal Mass Ejections: A Predictive Theoretical Model for Solar-type Stars
DOI: 10.3847/1538-4357/aa6f0e Bibcode: 2017ApJ...840..114C

Cranmer, Steven R.

Coronal mass ejections (CMEs) are eruptive events that cause a solar-type star to shed mass and magnetic flux. CMEs tend to occur together with flares, radio storms, and bursts of energetic particles. On the Sun, CME-related mass loss is roughly an order of magnitude less intense than that of the background solar wind. However, on other types of s…

2017 The Astrophysical Journal
SOHO 53
Chandra and JVLA Observations of HST Frontier Fields Cluster MACS J0717.5+3745
DOI: 10.3847/1538-4357/835/2/197 Bibcode: 2017ApJ...835..197V

Churazov, E.; Zitrin, A.; Rosati, P. +24 more

To investigate the relationship between thermal and non-thermal components in merger galaxy clusters, we present deep JVLA and Chandra observations of the HST Frontier Fields cluster MACS J0717.5+3745. The Chandra image shows a complex merger event, with at least four components belonging to different merging subclusters. Northwest of the cluster,…

2017 The Astrophysical Journal
eHST 53
Signatures of Nitrogen Chemistry in Hot Jupiter Atmospheres
DOI: 10.3847/2041-8213/aa97d4 Bibcode: 2017ApJ...850L..15M

Madhusudhan, Nikku; MacDonald, Ryan J.

Inferences of molecular compositions of exoplanetary atmospheres have generally focused on carbon, hydrogen, and oxygen-bearing molecules. Recently, additional absorption in Hubble Space Telescope Wide Field Camera 3 (WFC3) transmission spectra around 1.55 µm has been attributed to nitrogen-bearing chemical species: NH3 or HCN. Th…

2017 The Astrophysical Journal
eHST 53
Surface Gravities for 228 M, L, and T Dwarfs in the NIRSPEC Brown Dwarf Spectroscopic Survey
DOI: 10.3847/1538-4357/aa6338 Bibcode: 2017ApJ...838...73M

Kirkpatrick, J. Davy; Burgasser, Adam J.; Logsdon, Sarah E. +6 more

We combine 131 new medium-resolution (R ∼ 2000) J-band spectra of M, L, and T dwarfs from the Keck NIRSPEC Brown Dwarf Spectroscopic Survey (BDSS) with 97 previously published BDSS spectra to study surface-gravity-sensitive indices for 228 low-mass stars and brown dwarfs spanning spectral types M5-T9. Specifically, we use an established set of spe…

2017 The Astrophysical Journal
Gaia 53