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We cross-match objects from several different astronomical catalogs to determine the absolute proper proper motions of stars within the 30-arcmin radius fields of 115 Milky-Way globular clusters with the accuracy of 1--2~mas/yr. The proper…

Astrophysics of Galaxies · Physics 2018-06-13 A. A. Chemel , E. V. Glushkova , A. K. Dambis , A. S. Rastorguev , L. N. Yalyalieva

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 latitude | b | < 10 deg with an effective angular resolution of…

We present the results of a large-scale proper motion study of the central ~36'x16' of the Milky Way, based on our high angular resolution GALACTICNUCLEUS survey (epoch 2015) combined with the HST Paschen-alpha survey (epoch 2008). Our…

This study constitutes part of a larger effort aimed at better characterizing the Galactic globular clusters (GGCs) located towards the inner Milky Way bulge and disk. Here, we focus on internal kinematics of nine GGCs, obtained from…

Astrophysics of Galaxies · Physics 2021-01-06 Roger E. Cohen , Andrea Bellini , Mattia Libralato , Matteo Correnti , Thomas M. Brown , Jason S. Kalirai

The Milky Way, when viewed in the neutral hydrogen line emission, presents large structures called Galactic supershells (GSs). The origin of these structures is still a subject of debate. The most common scenario invoked is the combined…

Astrophysics of Galaxies · Physics 2019-04-10 L. A. Suad , C. F. Caiafa , S. Cichowolski , E. M. Arnal

We present a sample of 1148 ab-type RR Lyrae (RRLab) variables identified from Catalina Surveys Data Release 1, combined with SDSS DR8 and LAMOST DR4 spectral data. We firstly use a large sample of 860 Galactic halo RRLab stars and derive…

Astrophysics of Galaxies · Physics 2017-09-06 Iminhaji Ablimit , Gang Zhao

We study three processes that eject hypervelocity (>10^3 km/s) stars from the Galactic center: (i) close encounters of two single stars; (ii) tidal breakup of binary stars by the central black hole, as originally proposed by Hills; and…

Astrophysics · Physics 2008-11-26 Qingjuan Yu , Scott Tremaine

Typical stars in the Milky Way galaxy have velocities of hundreds of kilometres per second and experience gravitational accelerations of $\sim 10^{-10}$ m s$^{-2}$, resulting in velocity changes of a few centimetres per second over a…

Astrophysics of Galaxies · Physics 2019-09-18 Hamish Silverwood , Richard Easther

Outside of the known star clusters in the Galactic Center, a large number of evolved massive stars have been detected; but their origins remain uncertain. We present a spectroscopic study of eight such stars, based on new Gemini GNIRS and…

Astrophysics of Galaxies · Physics 2014-10-13 Hui Dong , Jon Mauerhan , Mark R. Morris , Q. Daniel Wang , Angela Cotera

We surveyed 291 MSX/2MASS infrared objects in the 7 x 2 deg area of the galactic center in the 43 GHz SiO J=1--0 v=1 and 2 maser lines, obtaining accurate radial velocities of 163 detected objects. The surveyed area is the region where the…

We present a three dimensional velocity analysis of Milky Way disk kinematics using LAMOST K giant stars and the GPS1 proper motion catalogue. We find that Galactic disk stars near the anticenter direction (in the range of Galactocentric…

Astrophysics of Galaxies · Physics 2018-04-03 Haifeng Wang , Martín López-Corredoira , Jeffrey L. Carlin , Licai Deng

Obtaining reliable distance estimates to gas clouds within the Milky Way is challenging in the absence of certain tracers. The kinematic distance approach has been used as an alternative, derived from the assumption of circular trajectories…

We present new results based on high-resolution observations of Sgr A West at the Galactic center with the VLA at 1.3 cm. We measured proper motions for 71 compact HII components. We also investigated radial velocities in the LSR velocity…

Astrophysics of Galaxies · Physics 2009-06-25 Jun-Hui Zhao , Mark R. Morris , W. M. Goss , Tao An

The goal of this paper is to demonstrate the outstanding quality of the second data release of the Gaia mission and its power for constraining many different aspects of the dynamics of the satellites of the Milky Way. We focus here on…

Direct dynamical mass measurements of stars with masses above 30 M${}_\odot$ are rare. This is the result of the low yield of the upper initial mass function and the limited number of such systems in eclipsing binaries. Long-period,…

Solar and Stellar Astrophysics · Physics 2021-08-04 M. Fabry , C. Hawcroft , A. J. Frost , L. Mahy , P. Marchant , J-B. Le Bouquin , H. Sana

Previous analyses of large databases of Milky Way stars have revealed the stellar disk of our Galaxy to be warped and that this imparts a strong signature on the kinematics of stars beyond the solar neighborhood. However, due to the…

Stars in the Galactic disc, including the Solar system, have deviated from their birth orbits and have experienced radial mixing and vertical heating. By performing hydrodynamical simulations of a galactic disc, we investigate how much…

Astrophysics of Galaxies · Physics 2023-06-07 Yusuke Fujimoto , Shu-ichiro Inutsuka , Junichi Baba

We infer the past orbit of the Sagittarius (Sgr) dwarf galaxy in the Milky Way halo by integrating backwards from its observed position and proper motions, including the effects of dynamical friction. Given measured proper motions, we show…

Astrophysics of Galaxies · Physics 2014-02-12 Sukanya Chakrabarti , Alice Quillen , Philip Chang , David Merritt

Recent observations with the James Webb Space Telescope (JWST) have revealed massive, evolved galaxies only a few hundred million years after the Big Bang, challenging standard cosmological models. To test the hypothesis that the Galactic…

Astrophysics of Galaxies · Physics 2025-09-16 G. S. Karapetian , L. E. Byzalov , M. A. Hovhannisyan , L. A. Mahtessian , A. P. Mahtessian

We have searched for the SiO J=1--0 v= 1 and 2 maser lines at ~ 43 GHz in 277 2MASS/MSX/IRAS sources off the Galactic plane (|b|> 3 deg), which resulted in 119 (112 new) detections. Among the new detections, are two very faint objects with…

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