Universidad Cat'olica del Norte

发表

Confirmation of the binary status of Chamaeleon Hα 2- a very young low-mass binary in Chamaeleon ,

Jena, H Germany, D. D. Astronom'ia, 2008, 0803.2897.

He II λ4686 EMISSION FROM THE MASSIVE BINARY SYSTEM IN η CAR: CONSTRAINTS TO THE ORBITAL ELEMENTS AND THE NATURE OF THE PERIODIC MINIMA

Western Michigan University, Astrophysics, Canada., 2016, The Astrophysical Journal.

Orbital motion of the young brown dwarf companion TWA 5 B

Jena, H Germany, D. D. Astronom'ia, 2010, 1005.1244.

Multiwavelength campaign on Mrk 509 - VI. HST/COS observations of the far-ultraviolet spectrum

Technion, University College London, Mullard Space Science Laboratory, 2011, 1107.0661.

Chemical abundances of giant stars in NGC 5053 and NGC 5634, two globular clusters associated with the Sagittarius dwarf Spheroidal galaxy?

Santiago, Strasbourg, France., 2015, 1505.01487.

NGTS-10b: the shortest period hot Jupiter yet discovered

Santiago, Cambridge, Astrophysics, 2019, Monthly Notices of the Royal Astronomical Society.

Near-infrared photometry of globular clusters towards the Galactic bulge: observations and photometric metallicity indicators

Brazil., Ufrgs, C. M. Bidin, 2016, 1609.07824.

Astrometric confirmation of young low-mass binaries and multiple systems in the Chamaeleon star-forming regions

Jena, Davis, Astrophysics, 2012, 1204.3332.

Direct evidence of a sub-stellar companion around CT Chamaeleontis

Jena, Astronomy, Gottingen, 2008, 0809.2812.

Multiwavelength campaign on Mrk 509 XV. A global modeling of the broad emission lines in the Optical, UV and X-ray bands

Esac, S. Paltani, Stsci, 2016, 1606.06579.

A new class of fossil fragments from the hierarchical assembly of the Galactic bulge

Liverpool John Moores University, H Germany, UK., 2020, Nature Astronomy.

The Distance to the Stars

Garching, Bochum, Warsaw, 2023, 2311.03310.

Variability of the coronal line region in NGC 4151

U. Oxford, U. Kentucky, Q. Belfast, 2015, 1501.02928.