Search Publications

Spectroscopy and Photometry of Multiple Populations along the Asymptotic Giant Branch of NGC 2808 and NGC 6121 (M4)
DOI: 10.3847/1538-4357/aa7852 Bibcode: 2017ApJ...843...66M

Milone, A. P.; Marino, A. F.; Bedin, L. R. +8 more

We present a photometric and spectroscopic study of multiple populations along the asymptotic giant branch (AGB) of the intermediate-metallicity globular clusters (GCs) NGC 2808 and NGC 6121 (M4). Chemical abundances of O, Na, Mg, Al, Si, Ca, Sc, Ti, V, Cr, Fe, Co, Ni, Zn, Y, and Ce in AGB stars from high-resolution FLAMES+UVES@VLT spectra are rep…

2017 The Astrophysical Journal
Gaia eHST 52
Evidence for multiple populations in the intermediate-age cluster Lindsay 1 in the SMC
DOI: 10.1093/mnrasl/slw179 Bibcode: 2017MNRAS.465L..39H

Rejkuba, M.; Bastian, N.; Lardo, C. +6 more

Lindsay 1 is an intermediate-age (≈8 Gyr) massive cluster in the Small Magellanic Cloud. Using VLT FORS2 spectra of 16 probable cluster members on the lower red giant branch of the cluster, we measure CN and CH band strengths (at ≃ 3883 and 4300 Å, respectively), along with carbon and nitrogen abundances and find that a sub-population of stars has…

2017 Monthly Notices of the Royal Astronomical Society
eHST 52
Near-infrared MOSFIRE Spectra of Dusty Star-forming Galaxies at 0.2 < z < 4
DOI: 10.3847/1538-4357/aa6cb1 Bibcode: 2017ApJ...840..101C

Casey, Caitlin M.; Sanders, D. B.; Capak, Peter +6 more

We present near-infrared and optical spectroscopic observations of a sample of 450 and 850 µm-selected dusty star-forming galaxies (DSFGs) identified in a 400 arcmin2 area in the COSMOS field. Thirty-one sources of the 114 targets were spectroscopically confirmed at 0.2< z< 4, identified primarily in the near-infrared with K…

2017 The Astrophysical Journal
eHST 52
Evolution of the reverberation lag in GX 339-4 at the end of an outburst
DOI: 10.1093/mnras/stx1649 Bibcode: 2017MNRAS.471.1475D

Ponti, G.; Tomsick, J. A.; Rodriguez, J. +13 more

We studied X-ray reverberation lags in the Black hole X-ray binary (BHXRB) GX 339-4 at the end of the 2014-2015 outburst. We analysed data from an XMM-Newton campaign covering the end of the transition from the soft to hard state, and the decrease of luminosity in the hard state. During all the observations we detected, at high frequencies, signif…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 52
Extended Main-sequence Turn-offs in Intermediate-age Star Clusters: Stellar Rotation Diminishes, but Does Not Eliminate, Age Spreads
DOI: 10.3847/1538-4357/aa7fb7 Bibcode: 2017ApJ...846...22G

Girardi, Léo; Goudfrooij, Paul; Correnti, Matteo

Extended main-sequence turn-off (eMSTO) regions are a common feature in color-magnitude diagrams of young- and intermediate-age star clusters in the Magellanic Clouds. The nature of eMSTOs remains debated in the literature. The currently most popular scenarios are extended star formation activity and ranges of stellar rotation rates. Here we study…

2017 The Astrophysical Journal
eHST 51
A search for sterile neutrinos with the latest cosmological observations
DOI: 10.1140/epjc/s10052-017-4986-3 Bibcode: 2017EPJC...77..418F

Feng, Lu; Zhang, Jing-Fei; Zhang, Xin

We report the result of a search for sterile neutrinos with the latest cosmological observations. Both cases of massless and massive sterile neutrinos are considered in the ΛCDM cosmology. The cosmological observations used in this work include th…

2017 European Physical Journal C
Planck 51
Constraints on the Lyman continuum escape fraction for faint star-forming galaxies
DOI: 10.1093/mnras/stx477 Bibcode: 2017MNRAS.468..389J

Tozzi, P.; Balestra, I.; Rosati, P. +6 more

Star-forming galaxies have long been considered the dominant sources of the cosmic ultraviolet background radiation at early epochs. However, observing and characterizing the galaxy population with significant ionizing emission have proven to be challenging. In particular, the fraction of ionizing radiation that escapes the local environment to th…

2017 Monthly Notices of the Royal Astronomical Society
eHST 51
SNR 1E 0102.2-7219 as an X-ray calibration standard in the 0.5-1.0 keV bandpass and its application to the CCD instruments aboard Chandra, Suzaku, Swift and XMM-Newton
DOI: 10.1051/0004-6361/201628824 Bibcode: 2017A&A...597A..35P

Miller, Eric D.; Haberl, Frank; Plucinsky, Paul P. +4 more

Context. The flight calibration of the spectral response of charge-coupled device (CCD) instruments below 1.5 keV is difficult in general because of the lack of strong lines in the on-board calibration sources typically available. This calibration is also a function of time due to the effects of radiation damage on the CCDs and/or the accumulation…

2017 Astronomy and Astrophysics
Suzaku XMM-Newton 51
Dissecting the extended main-sequence turn-off of the young star cluster NGC 1850
DOI: 10.1093/mnras/stx010 Bibcode: 2017MNRAS.467.3628C

Bellini, Andrea; Goudfrooij, Paul; Puzia, Thomas H. +2 more

We use the Wide Field Camera 3 onboard the Hubble Space Telescope to obtain deep, high-resolution photometry of the young (∼100 Myr) star cluster NGC 1850 in the Large Magellanic Cloud. We analyse the cluster colour-magnitude diagram (CMD) and find that it hosts an extended main-sequence turn-off (MSTO) and a double main sequence (MS). We demonstr…

2017 Monthly Notices of the Royal Astronomical Society
eHST 51
Revealing the structure of the outer disks of Be stars
DOI: 10.1051/0004-6361/201629932 Bibcode: 2017A&A...601A..74K

Carciofi, A. C.; Štefl, S.; Vieira, R. G. +9 more

Context. The structure of the inner parts of Be star disks (≲ 20 stellar radii) is well explained by the viscous decretion disk (VDD) model, which is able to reproduce the observable properties of most of the objects studied so far. The outer parts, on the other hand, are not observationally well-explored, as they are observable only at radio wave…

2017 Astronomy and Astrophysics
IUE 51