Search Publications

ISO-ChaI 52: a weakly accreting young stellar object with a dipper light curve
DOI: 10.1051/0004-6361/202038157 Bibcode: 2020A&A...639L...8F

Fedele, D.; Alcalá, J. M.; Manara, C. F. +6 more

We report the discovery of periodic dips in the multiband light curve of ISO-ChaI 52, a young stellar object in the Chamaeleon I dark cloud. This is one of the peculiar objects that display very low or negligible accretion in their UV continuum and spectral lines, although they present a remarkable infrared excess emission characteristic of optica…

2020 Astronomy and Astrophysics
Gaia 4
Lessons on early structure formation from a mature galaxy cluster observed at cosmic noon
DOI: 10.1093/mnras/staa1307 Bibcode: 2020MNRAS.495.1700L

Bromm, Volker; Liu, Boyuan; Schauer, Anna T. P.

We demonstrate a new approach of indirectly constraining both early star and structure formation via mature galaxy clusters at cosmic noon (z ∼ 2), using the cluster XLSSC 122 as an example. With the standard Press Schechter formalism, we infer a rapid evolution of the star formation efficiency (the ratio of stellar to halo mass) from 10-4

2020 Monthly Notices of the Royal Astronomical Society
eHST 4
The Energetic Thermonuclear Bursts in SAX J1712.6-3739
DOI: 10.3847/1538-4357/abb76f Bibcode: 2020ApJ...903...37L

Lin, Jie; Yu, Wenfei

The neutron star low-mass X-ray binary SAX J1712.6-3739 is known for its long and hard thermonuclear X-ray bursts from previous observations. Its thermonuclear bursts are so distinct as they can last for tens of minutes, as seen with Swift/BAT (E > 15 keV). To explore the origin of these extreme bursts and the nature of SAX J1712.6-3739, we ana…

2020 The Astrophysical Journal
INTEGRAL 4
Study of Star-Forming Regions in the Peculiar Galaxies NGC 660, NGC 1512, NGC 4395, and NGC 4618
DOI: 10.1134/S199034132003013X Bibcode: 2020AstBu..75..234S

Smirnova, K. I.; Wiebe, D. S.; Moiseev, A. V. +1 more

—The star-forming regions (SFRs) in the peculiar galaxies NGC 660, NGC 1512, NGC 4395 and NGC 4618 are studied. The relationships between such characteristics of star forming regions as UV, near- and far-IR fluxes, as well as in the Hα and HI lines, surface brightness in these ranges, and the scatter of the radial velocities of ionized and neutral…

2020 Astrophysical Bulletin
Herschel 4
The Dynamics of the Magnetic-field-free Cavity around Comets
DOI: 10.3847/1538-4357/ab6e69 Bibcode: 2020ApJ...891..112N

Nemeth, Z.

The diamagnetic cavity is the innermost region of the magnetosphere of an active comet, from which the magnetic field is expelled by the outflowing matter. This phenomenon, first detected around comet 1P/Halley, was extensively studied recently by the Rosetta comet chaser mission. Rosetta observed a surprisingly large diamagnetic cavity around com…

2020 The Astrophysical Journal
Rosetta 4
Gas kinematics of key prebiotic molecules in GV Tau N revealed with an ALMA, PdBI, and Herschel synergy
DOI: 10.1093/mnras/staa1919 Bibcode: 2020MNRAS.496.5330F

Pilleri, P.; Fuente, A.; Rivière-Marichalar, P. +4 more

A large effort has been made to detect warm gas in the planet formation zone of circumstellar discs using space and ground-based near-infrared facilities. GV Tau N, the most obscured component of the GV Tau system, is an outstanding source, being one of the first targets detected in HCN and the only one detected in CH4 so far. Although …

2020 Monthly Notices of the Royal Astronomical Society
Gaia 4
The Herschel SPIRE Fourier Transform Spectrometer Spectral Feature Finder - III. Line identification and off-axis spectra
DOI: 10.1093/mnras/staa1613 Bibcode: 2020MNRAS.496.4906B

Valtchanov, I.; Spencer, L. D.; Hopwood, R. +5 more

The European Space Agency Herschel Spectral and Photometric Imaging Receiver (SPIRE) Fourier Transform Spectrometer (FTS) Spectral Feature Finder (FF) project is an automated spectral feature fitting routine developed within the SPIRE instrument team to extract all prominent spectral features from all publicly available SPIRE FTS observations. We …

2020 Monthly Notices of the Royal Astronomical Society
Herschel 4
Spatial distribution of exoplanet candidates based on Kepler and Gaia data
DOI: 10.1051/0004-6361/201936692 Bibcode: 2020A&A...635A.191M

Budaj, J.; Maliuk, A.

Context. Surveying the spatial distribution of exoplanets in the Galaxy is important for improving our understanding of planet formation and evolution.
Aims: We aim to determine the spatial gradients of exoplanet occurrence in the Solar neighbourhood and in the vicinity of open clusters.
Methods: We combined Kepler and Gaia DR2 data for …

2020 Astronomy and Astrophysics
Gaia 4
WIYN Open Cluster Study. LXXXI. Caught in the Act? The Peculiar Red Giant NGC 2243-W2135
DOI: 10.3847/1538-3881/ab9ca2 Bibcode: 2020AJ....160...75A

Twarog, Bruce A.; Anthony-Twarog, Barbara J.; Deliyannis, Constantine P.

High-dispersion spectra for giants through turnoff stars in the Li 6708 Å region have been obtained and analyzed in the old, metal-deficient open cluster, NGC 2243. When combined with high-dispersion data from other surveys, the cluster is found to contain a uniquely peculiar star at the luminosity level of the red clump. The giant is the reddest …

2020 The Astronomical Journal
Gaia 4
Latitudinal distribution of solar coronal active regions
DOI: 10.1016/j.asr.2019.11.028 Bibcode: 2020AdSpR..65.1321M

Chargeishvili, B. B.; Maghradze, D. A.; Japaridze, D. R. +3 more

We studied the cyclic evolution of the latitudinal distribution of solar coronal active regions based on daily images from SOHO EIT for the period 1995-2017. Fully automated software was used, which included the following steps: initial preparation of images in the data series, normalization of histograms and correction of limb brightening, segmen…

2020 Advances in Space Research
SOHO 3