Search Publications

Haumea's thermal emission revisited in the light of the occultation results
DOI: 10.1016/j.icarus.2018.11.011 Bibcode: 2019Icar..334...39M

Fornasier, S.; Lellouch, E.; Marton, G. +9 more

A recent multi-chord occultation measurement of the dwarf planet (136108) Haumea (Ortiz et al., 2017) revealed an elongated shape with the longest axis comparable to Pluto's mean diameter. The chords also indicate a ring around Haumea's equatorial plane, where its largest moon, Hi'iaka, is also located. The Haumea occultation size estimate (size o…

2019 Icarus
Herschel 13
2 mm GISMO Observations of the Galactic Center. I. Dust Emission
DOI: 10.3847/1538-4357/ab451c Bibcode: 2019ApJ...885...71A

Morris, Mark R.; Staguhn, Johannes; Gonzalez-Quiles, Junellie +5 more

The central molecular zone, covering the inner ∼1° of the Galactic plane has been mapped at 2 mm using the Goddard-IRAM Superconducting 2-Millimeter Observer (GISMO) bolometric camera on the 30 m IRAM telescope. The 21″ resolution maps show abundant emission from cold molecular clouds, from star-forming regions, and from one of the Galactic center…

2019 The Astrophysical Journal
Herschel 13
Characterizing dynamical stages of open clusters located in the Sagittarius spiral arm
DOI: 10.1093/mnras/stz1709 Bibcode: 2019MNRAS.488.1635A

Maia, F. F. S.; Angelo, M. S.; Dias, W. S. +1 more

The study of dynamical properties of Galactic open clusters (OCs) is a fundamental prerequisite for the comprehension of their dissolution processes. In this work, we characterized 12 OCs, namely: Collinder 258, NGC 6756, Czernik 37, NGC 5381, Ruprecht 111, Ruprecht 102, NGC 6249, Basel 5, Ruprecht 97, Trumpler 25, ESO 129-SC32, and BH 150, projec…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 13
Hunting for brown dwarfs in the globular cluster M4: second epoch HST NIR observations
DOI: 10.1093/mnras/stz996 Bibcode: 2019MNRAS.486.2254D

Knigge, C.; Bedin, L. R.; Rich, R. M. +5 more

We present an analysis of the second epoch Hubble Space TelescopeWide Field Camera 3 F110W near-infrared (NIR) imaging data of the globular cluster M 4. The new data set suggests that one of the previously suggested four brown dwarf candidates in this cluster is indeed a high-probability cluster member. The position of this object in the NIR colou…

2019 Monthly Notices of the Royal Astronomical Society
eHST 13
Neutron Stars and Black Holes in the Small Magellanic Cloud: The SMC NuSTAR Legacy Survey
DOI: 10.3847/1538-4357/ab3f32 Bibcode: 2019ApJ...884....2L

Haberl, F.; Lehmer, B. D.; Hornschemeier, A. E. +18 more

We present a source catalog from the first deep hard X-ray (E > 10 keV) survey of the Small Magellanic Cloud (SMC), the Nuclear Spectroscopic Telescope Array (NuSTAR) Legacy Survey of the SMC. We observed three fields, for a total exposure time of 1 Ms, along the bar of this nearby star-forming galaxy. Fields were chosen for their young stellar…

2019 The Astrophysical Journal
XMM-Newton 13
Tentative detection of the circumgalactic medium of the isolated low-mass dwarf galaxy WLM
DOI: 10.1093/mnras/stz2563 Bibcode: 2019MNRAS.490..467Z

McQuinn, Kristen B. W.; Lockman, Felix J.; Fox, Andrew J. +7 more

We report a tentative detection of the circumgalactic medium (CGM) of Wolf-Lundmark-Melotte (WLM), an isolated, low-mass (logM*/M ≈ 7.6), dwarf irregular galaxy in the Local Group (LG). We analyse an HST/COS archival spectrum of a quasar sightline (PHL2525), which is 45 kpc (0.5 virial radius) from WLM and close to the Magel…

2019 Monthly Notices of the Royal Astronomical Society
eHST 13
Co-spatial UV-optical HST/STIS spectra of six planetary nebulae: nebular and stellar properties
DOI: 10.1093/mnras/sty2517 Bibcode: 2019MNRAS.482..278M

Corradi, Romano L. M.; Balick, Bruce; Shaw, Richard A. +4 more

This paper represents the conclusion of a project that had two main goals: (1) to investigate to what extent planetary nebulae (PNe) are chemically homogeneous; and (2) to provide physical constraints on the central star properties of each PN. We accomplished the first goal by using HST/STIS spectra to measure the abundances of seven elements in n…

2019 Monthly Notices of the Royal Astronomical Society
Gaia eHST 13
A combined X-ray, optical, and radio view of the merging galaxy cluster MACS J0417.5-1154
DOI: 10.1093/mnras/sty2937 Bibcode: 2019MNRAS.482.5093P

Simionescu, A.; Limousin, M.; Raychaudhury, S. +3 more

We present a comprehensive multiwavelength analysis of the merging galaxy cluster MACS J0417.5-1154 at a redshift of z = 0.44, using available images red obtained with Chandra in X-ray, Subaru, Hubble Space Telescope (HST) in optical, Giant Metrewave Radio Telescope (GMRT) in radio, and Bolocam at 2.1 mm wavelength. This is an example of a complex…

2019 Monthly Notices of the Royal Astronomical Society
eHST 13
Evidence of New Magnetic Transitions in Late-type Dwarfs from Gaia DR2
DOI: 10.3847/1538-4357/ab1aa2 Bibcode: 2019ApJ...877..157L

Spada, Federico; Distefano, Elisa; Lanzafame, Alessandro C. +1 more

The second Gaia data release contains the identification of 147,535 low-mass (≲ 1.4 {M}) rotational modulation variable candidates on (or close to) the main sequence, together with their rotation period and modulation amplitude. The richness, the period and amplitude range, and the photometric precision of this sample make it possible…

2019 The Astrophysical Journal
Gaia 13
Thermal Emission and Magnetic Beaming in the Radio and X-Ray Mode-switching PSR B0943+10
DOI: 10.3847/1538-4357/aafac7 Bibcode: 2019ApJ...872...15R

Mereghetti, Sandro; Turolla, Roberto; Potekhin, Alexander Y. +3 more

PSR B0943+10 is a mode-switching radio pulsar characterized by two emission modes with different radio and X-ray properties. Previous studies, based on simple combinations of blackbody and power-law models, showed that its X-ray flux can be decomposed in a pulsed thermal plus an unpulsed nonthermal components. However, if PSR B0943+10 is a nearly …

2019 The Astrophysical Journal
XMM-Newton 12