Search Publications

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
Seismic modelling of early B-type pulsators observed by BRITE - I. θ Ophiuchi
DOI: 10.1093/mnras/stz639 Bibcode: 2019MNRAS.485.3544W

Moffat, Anthony F. J.; Pablo, Herbert; Walczak, Przemysław +8 more

We analyse time-series observations from the BRITE-Constellation of the well-known β Cephei type star θ Ophiuchi. Seven previously known frequencies were confirmed and 19 new frequency peaks were detected. In particular, high-order g modes, typical for the SPB (Slowly Pulsating B-type star) pulsators, are uncovered. These low-frequency modes are a…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 25
A search for gravitationally lensed quasars and quasar pairs in Pan-STARRS1: spectroscopy and sources of shear in the diamond 2M1134-2103
DOI: 10.1093/mnras/stz1142 Bibcode: 2019MNRAS.486.4987R

Fassnacht, Christopher D.; Chen, Geoff C. -F.; Nelson, George J. +4 more

We present results of a systematic search for gravitationally lensed quasars in Pan-STARRS1. Our final sample of candidates comprises of 91 systems, not including 25 rediscovered lensed quasars and quasar pairs. In the absence of spectroscopy to verify the lensing nature of the candidates, the main sources of contaminants are likely to be quasar p…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 25
Resolved scaling relations and metallicity gradients on sub-kiloparsec scales at z ≈ 1
DOI: 10.1093/mnras/stz2114 Bibcode: 2019MNRAS.489..224P

Mahler, G.; Richard, J.; Nanayakkara, T. +9 more

The existence of a spatially resolved star-forming main sequence (rSFMS) and a spatially resolved mass-metallicity relation (rMZR) is now well established for local galaxies. Moreover, gradients with metallicity decreasing with radius seem to be common in local disc galaxies. These observations suggest that galaxy formation is a self-regulating pr…

2019 Monthly Notices of the Royal Astronomical Society
eHST 25
Interstellar polarization and extinction in the Local Bubble and the Gould Belt
DOI: 10.1093/mnras/sty2978 Bibcode: 2019MNRAS.483..299G

Gontcharov, George A.; Mosenkov, Aleksandr V.

We analyse an all-sky compilation of 13 data sources with optical interstellar linear polarization for 3871 Gaia DR2 and Hipparcos stars within 500 pc, which do not exhibit a considerable intrinsic polarization. These data are analysed together with five 3D maps and models of the reddening E(B - V). We consider variations of the polarization degre…

2019 Monthly Notices of the Royal Astronomical Society
Gaia Hipparcos 25
TOI-150b and TOI-163b: two transiting hot Jupiters, one eccentric and one inflated, revealed by TESS near and at the edge of the JWST CVZ
DOI: 10.1093/mnras/stz2433 Bibcode: 2019MNRAS.490.1094K

Henning, Thomas; Kürster, Martin; Jordán, Andrés +51 more

We present the discovery of TYC9191-519-1b (TOI-150b, TIC 271893367) and HD271181b (TOI-163b, TIC 179317684), two hot Jupiters initially detected using 30-min cadence Transiting Exoplanet Survey Satellite (TESS) photometry from Sector 1 and thoroughly characterized through follow-up photometry (CHAT, Hazelwood, LCO/CTIO, El Sauce, TRAPPIST-S), hig…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 25
Mass loss via solar wind and coronal mass ejections during solar cycles 23 and 24
DOI: 10.1093/mnras/stz1001 Bibcode: 2019MNRAS.486.4671M

Wang, Yuming; Liu, Rui; Srivastava, Nandita +3 more

Similar to the Sun, other stars shed mass and magnetic flux via ubiquitous quasi-steady wind and episodic stellar coronal mass ejections (CMEs). We investigate the mass loss rate via solar wind and CMEs as a function of solar magnetic variability represented in terms of sunspot number and solar X-ray background luminosity. We estimate the contribu…

2019 Monthly Notices of the Royal Astronomical Society
SOHO 25
Early science with the Large Millimetre Telescope: An LMT/AzTEC 1.1 mm Survey of dense cores in the Monoceros R2 giant molecular cloud
DOI: 10.1093/mnras/sty3107 Bibcode: 2019MNRAS.483..407S

Wilson, G. W.; Schloerb, F. P.; Luna, A. +7 more

We present a 1.1 mm census of dense cores in the Mon R2 giant molecular cloud with the AzTEC instrument on the Large Millimetre Telescope. We detect 295 cores (209 starless and 86 with protostars) in a two square degree shallow survey. We also carry out a deep follow-up survey of nine regions with low to intermediate (3 < AV < 7) …

2019 Monthly Notices of the Royal Astronomical Society
Herschel 25
Extraction of globular clusters members with Gaia DR2 astrometry
DOI: 10.1093/mnras/stz1879 Bibcode: 2019MNRAS.488.3024B

Bustos Fierro, Iván H.; Calderón, J. H.

In this work, we present a method to identify possible members of globular clusters using data from Gaia DR2. The method consists of two stages: the first one based on a clustering algorithm, and the second one based on the analysis of the projected spatial distribution of stars with different proper motions. In order to confirm that the clusters …

2019 Monthly Notices of the Royal Astronomical Society
Gaia 25