Search Publications

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
Infrared Selection of Obscured Active Galactic Nuclei in the COSMOS Field
DOI: 10.3847/1538-4365/aa97da Bibcode: 2017ApJS..233...19C

Kartaltepe, Jeyhan S.; Tang, Ji-Jia; Juneau, Stéphanie +13 more

We present a study of the connection among black hole accretion, star formation, and galaxy morphology at z≤slant 2.5. We focus on active galactic nuclei (AGNs) selected by their mid-IR power-law emission. By fitting optical to far-IR photometry with state-of-the-art spectral energy distribution (SED) techniques, we derive stellar masses, star for…

2017 The Astrophysical Journal Supplement Series
eHST 53
Evidence of sub-surface energy storage in comet 67P from the outburst of 2016 July 03
DOI: 10.1093/mnras/stx2386 Bibcode: 2017MNRAS.469S.606A

Langevin, Y.; Jorda, L.; Lamy, P. L. +67 more

On 2016 July 03, several instruments onboard ESA's Rosetta spacecraft detected signs of an outburst event on comet 67P, at a heliocentric distance of 3.32 au from the Sun, outbound from perihelion. We here report on the inferred properties of the ejected dust and the surface change at the site of the outburst. The activity coincided with the local…

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 53
Conjoined constraints on modified gravity from the expansion history and cosmic growth
DOI: 10.1103/PhysRevD.96.063517 Bibcode: 2017PhRvD..96f3517B

Nesseris, Savvas; Basilakos, Spyros

In this paper we present conjoined constraints on several cosmological models from the expansion history H (z ) and cosmic growth f σ8. The models we study include the CPL w0wa parametrization, the holographic dark energy (HDE) model, the time-varying vacuum (ΛtCDM ) model, the Dvali, Gabadadze and Porra…

2017 Physical Review D
Planck 53
Partial redistribution in 3D non-LTE radiative transfer in solar-atmosphere models
DOI: 10.1051/0004-6361/201629086 Bibcode: 2017A&A...597A..46S

Leenaarts, Jorrit; Sukhorukov, Andrii V.

Context. Resonance spectral lines such as H I Ly α, Mg II H&K, and Ca II H&K that form in the solar chromosphere, are influenced by the effects of 3D radiative transfer as well as partial redistribution (PRD). So far no one has modeled these lines including both effects simultaneously owing to the high computing demands of existing algorit…

2017 Astronomy and Astrophysics
IRIS 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
Herschel -ATLAS: revealing dust build-up and decline across gas, dust and stellar mass selected samples - I. Scaling relations
DOI: 10.1093/mnras/stw2501 Bibcode: 2017MNRAS.464.4680D

Ivison, R. J.; Baes, M.; Baker, A. J. +19 more

We present a study of the dust, stars and atomic gas (H I) in an H I-selected sample of local galaxies (z < 0.035) in the Herschel Astrophysical Terahertz Large Area Survey fields. This H I-selected sample reveals a population of very high gas fraction (>80 per cent), low stellar mass sources that appear to be in the earliest stages of their…

2017 Monthly Notices of the Royal Astronomical Society
Herschel 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
Detection of nanoflare-heated plasma in the solar corona by the FOXSI-2 sounding rocket
DOI: 10.1038/s41550-017-0269-z Bibcode: 2017NatAs...1..771I

Krucker, Säm; Narukage, Noriyuki; Glesener, Lindsay +4 more

The processes that heat the solar and stellar coronae to several million kelvins, compared with the much cooler photosphere (5,800 K for the Sun), are still not well known1. One proposed mechanism is heating via a large number of small, unresolved, impulsive heating events called nanoflares2. Each event would heat and cool qu…

2017 Nature Astronomy
Hinode 53