Search Publications

Evidence for a Massive Warm-Hot Circumgalactic Medium around NGC 3221
DOI: 10.3847/1538-4357/ab48df Bibcode: 2019ApJ...885..108D

Nicastro, Fabrizio; Mathur, Smita; Gupta, Anjali +3 more

We report a 3.4σ detection of the warm-hot, massive, extended circumgalactic medium (CGM) around an L star-forming spiral galaxy NGC 3221, using deep Suzaku observations. The temperature of the gas is 106.1 K, comparable to that of the Milky Way CGM. The spatial extent of the gas is at least 150 kpc. For a β-model of densit…

2019 The Astrophysical Journal
Suzaku 25
Linear bias forecasts for emission line cosmological surveys
DOI: 10.1093/mnras/stz1204 Bibcode: 2019MNRAS.486.5737M

Merson, Alexander; Smith, Alex; Benson, Andrew +2 more

We forecast the linear bias for Hα-emitting galaxies at high redshift. To simulate a Euclid-like and a WFIRST-like survey, we place galaxies into a large-volume dark matter halo lightcone by sampling a library of luminosity-dependent halo occupation distributions (HODs), which is constructed using a physically motivated galaxy formation model. We …

2019 Monthly Notices of the Royal Astronomical Society
eHST 25
A Gaia view of the two OB associations Cygnus OB2 and Carina OB1: the signature of their formation process
DOI: 10.1093/mnras/stz2548 Bibcode: 2019MNRAS.490..440L

Lim, Beomdu; Nazé, Yaël; Gosset, Eric +1 more

OB associations are the prime star-forming sites in galaxies. However, the detailed formation process of such stellar systems still remains a mystery. In this context, identifying the presence of substructures may help in tracing the footprints of their formation process. Here, we present a kinematic study of the two massive OB associations Cygnus…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 25
The compact multiple system HIP 41431
DOI: 10.1093/mnras/stz1510 Bibcode: 2019MNRAS.487.4631B

Molnár, L.; Latham, D. W.; Tokovinin, A. +4 more

The nearby (50 pc) K7V dwarf HIP 41431 (EPIC 212096658) is a compact three-tier hierarchy. Three K7V stars with similar masses, from 0.61 to 0.63 solar, make a triple-lined spectroscopic system where the inner binary with a period of 2.9 d is eclipsing, and the outer companion on a 59-d orbit exerts strong dynamical influence revealed by the eclip…

2019 Monthly Notices of the Royal Astronomical Society
Gaia Hipparcos 25
K2-290: a warm Jupiter and a mini-Neptune in a triple-star system
DOI: 10.1093/mnras/stz139 Bibcode: 2019MNRAS.484.3522H

Kuzuhara, M.; Alonso, R.; Deeg, H. +41 more

We report the discovery of two transiting planets orbiting K2-290 (EPIC 249624646), a bright (V = 11.11) late F-type star residing in a triple-star system. It was observed during Campaign 15 of the K2 mission, and in order to confirm and characterize the system, follow-up spectroscopy and AO imaging were carried out using the FIES, HARPS, HARPS-N,…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 25
Long-term evolutions of the cyclotron line energies in Her X-1, Vela X-1, and Cen X-3 as observed with Swift/BAT
DOI: 10.1093/mnras/stz264 Bibcode: 2019MNRAS.484.3797J

Santangelo, A.; Ducci, L.; Zhang, S. +3 more

We study the long-term evolution of the centroid energy of cyclotron lines - often referered to as cyclotron resonance scattering features (CRSFs) - in Her X-1, Vela X-1, and Cen X-3, using survey observations of the Burst Alert Telescope onboard Swift. We find a significant decrease of the fundamental CRSF energy in Her X-1 and the first harmonic…

2019 Monthly Notices of the Royal Astronomical Society
INTEGRAL 25
Solar wind charge exchange in cometary atmospheres. III. Results from the Rosetta mission to comet 67P/Churyumov-Gerasimenko
DOI: 10.1051/0004-6361/201834881 Bibcode: 2019A&A...630A..37S

Alho, Markku; Simon Wedlund, Cyril; Nilsson, Hans +12 more

Context. Solar wind charge-changing reactions are of paramount importance to the physico-chemistry of the atmosphere of a comet. The ESA/Rosetta mission to comet 67P/Churyumov-Gerasimenko (67P) provides a unique opportunity to study charge-changing processes in situ.
Aims: To understand the role of these reactions in the evolution of the sola…

2019 Astronomy and Astrophysics
Rosetta 25
Possible Evidence for Cosmic-Ray Acceleration in the Type Ia SNR RCW 86: Spatial Correlation between TeV Gamma-Rays and Interstellar Atomic Protons
DOI: 10.3847/1538-4357/ab108f Bibcode: 2019ApJ...876...37S

Rowell, G.; Fukui, Y.; Mitsuishi, I. +13 more

We present a detailed morphological study of TeV gamma-rays, synchrotron radiation, and interstellar gas in the young Type Ia supernova remnant (SNR) RCW 86. We find that the interstellar atomic gas shows good spatial correlation with the gamma-rays, indicating that the TeV gamma-rays from RCW 86 are likely predominantly of hadronic origin. In con…

2019 The Astrophysical Journal
XMM-Newton 25
Milky Way Tomography with the SkyMapper Southern Survey. I. Atmospheric Parameters and Distances of One Million Red Giants
DOI: 10.3847/1538-4365/ab1f72 Bibcode: 2019ApJS..243....7H

Wolf, C.; Wang, H. -F.; Huang, Y. +7 more

Accurate determinations of atmospheric parameters (effective temperature T eff, surface gravity log g, and metallicity [Fe/H]) and distances for large complete samples are of vital importance for various Galactic studies. We have developed a photometric method to select red giant stars and estimate their atmospheric parameters from the …

2019 The Astrophysical Journal Supplement Series
Gaia 25
The W UMa binaries USNO-A2.0 1350-17365531, V471 Cas, V479 Lac and V560 Lac: light curve solutions and global parameters based on Gaia distances
DOI: 10.1088/1674-4527/19/1/14 Bibcode: 2019RAA....19...14K

Popov, Velimir A.; Petrov, Nikola I.; Kjurkchieva, Diana P. +1 more

We present photometric observations in Sloan filters g‧, i‧ of the eclipsing W UMa stars USNO-A2.0 1350-17365531, V471 Cas, V479 Lac and V560 Lac. The sinusoidal-like O - C diagram of V471 Cas indicates the presence of a third body with mass 0.12 M (a red dwarf) at distance 897 R . The O - C diagram of V479 Lac reveals a p…

2019 Research in Astronomy and Astrophysics
Gaia 25