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HCN, HNC, H13CN & HC3N of Galactic Center map. II.
We report a statistical analysis exploring the origin of the overall low star formation efficiency (SFE) of the Galactic central molecular zone (CMZ) and the SFE diversity among... -
Radio continuum param. of Galactic HII regions
Sgr E is a massive star formation complex found toward the Galactic center that consists of numerous discrete, compact HII regions. It is located at the intersection between the... -
Abundances and ages of stars in the Milky Way bulge
The age and chemical characteristics of the Galactic bulge link to the formation and evolutionary history of the Galaxy. Data-driven methods and large surveys enable stellar... -
Gas structure comparison; NGC 253 and Milky Way
We compare molecular gas properties in the starbursting center of NGC253 and the Milky Way Galactic center (GC) on scales of ~1-100pc using dendrograms and resolution-, area-,... -
1482 Gaussian clumps in the Central Molecular Zone
We carry out a systematic study of the density structure of gas in the Central Molecular Zone (CMZ) in the Galactic center by extracting clumps from the APEX Telescope Large... -
Kinematic structure of the Galactic Center S cluster
We present a detailed analysis of the kinematics of 112 stars that mostly comprise the high-velocity S cluster and orbit the supermassive black hole Sgr A* at the center of the... -
ALMA obs. of massive clouds in the CMZ
We report Atacama Large Millimeter/submillimeter Array (ALMA) Band 6 continuum observations of 2000au resolution toward four massive molecular clouds in the Central Molecular... -
VVV survey microlensing events; -3.7<b{<}-3.9{deg}
We search for microlensing events in fields along the Galactic minor axis, ranging from the Galactic center to -3.7{deg}<b<3.9{deg} using the VISTA Variables in the Via... -
Keck/NIRC2 obs. of the Galactic Center
Precision measurements of the stars in short-period orbits around the supermassive black hole at the Galactic Center are now being used to constrain general relativistic... -
Molecular cloud cores in the GC 50km/s cloud
The Galactic center 50km/s molecular cloud (50MC) is the most remarkable molecular cloud in the Sagittarius A region. This cloud is a candidate for the massive star formation... -
Catalog of 563 stars in the Galactic Center
We present an ~11.5yr adaptive optics (AO) study of stellar variability and search for eclipsing binaries in the central ~0.4pc (~10") of the Milky Way nuclear star cluster. We... -
RR Lyrae cand. in the Galactic Center
Deep near-IR images from the VISTA Variables in the Via Lactea (VVV) Survey were used to search for RR Lyrae stars within 100 arcmin from the Galactic Center. A large sample of... -
Spitzer, VLT and Keck NIR light curves of SgrA*
Sagittarius A (Sgr A) is the variable radio, near-infrared (NIR), and X-ray source associated with accretion onto the Galactic center black hole. We present an analysis of the... -
Sgr A* 1.3mm VLBI observations with the EHT in 2013
We report results from very long baseline interferometric (VLBI) observations of the supermassive black hole in the Galactic center, Sgr A, at 1.3mm (230GHz). The observations... -
Spitzer/IRS observations of the Galactic Center
It has long been shown that the extreme ultraviolet spectrum of the ionizing stars of HII regions can be estimated by comparing the observed line emission to detailed models. In... -
Compact clouds in a sensitive GBT HI survey
We present the results of a new sensitive survey of neutral hydrogen above and below the Galactic Center with the Green Bank Telescope. The observations extend up to Galactic... -
16yrs of radial velocity measurements of S0-2
The star S0-2, which orbits the supermassive black hole (SMBH) in our Galaxy with a period of 16 years, provides the strongest constraint on both the mass of the SMBH and the... -
First Fermi-LAT Inner Galaxy point source catalog
The Fermi Large Area Telescope (LAT) has provided the most detailed view to date of the emission toward the Galactic center (GC) in high-energy {gamma}-rays. This paper... -
Galactic center: high-PM stars magnitude analysis
The Milky Way's central parsec is a highly extinguished region with a population of high-proper-motion stars. We have tracked 145 stars for ~10yr at wavelengths between 1 and... -
Period variations of 32 contact binaries
We present detailed analyses of updated eclipse timing diagrams for 32 contact binary merger candidates in the Galactic bulge. The photometric data was obtained from 2016 to...