English
Related papers

Related papers: To the Galactic Virial Radius with Hyper Suprime-C…

200 papers

Blue horizontal-branch (BHB) stars are ideal tracers for mapping the structure of Galactic stellar halo. Traditionally, BHB sample stars are built from large-scale spectroscopic surveys utilizing their spectral features, however, the…

Astrophysics of Galaxies · Physics 2025-05-07 Guozhen Hu , Yang Huang , Wenyuan Cui , Tao Wang , Kai Xiao , Ruifeng Shi , Jie Ju , Bowen Huang , Chunyan Li , Zhicun Liu , Xiaolong Wang , Changqing Luo

We identify new structures in the halo of the Milky Way Galaxy from positions, colors and magnitudes of five million stars detected in the Sloan Digital Sky Survey. Most of these stars are within 1.26 degrees of the celestial equator. We…

As a major component of the LAMOST Galactic surveys, the LAMOST Spectroscopic Survey of the Galactic Anti-center (LSS-GAC) will survey a significant volume of the Galactic thin/thick disks and halo in a contiguous sky area of ~…

We describe a major survey of the Milky Way halo designed to test for kinematic substructure caused by destruction of accreted satellites. We use the Washington photometric system to identify halo stars efficiently for spectroscopic…

We present the first results from our survey of stellar substructure in the outskirts of M31 using the Advanced Camera for Surveys (ACS) on board the Hubble Space Telescope. We discuss the stellar populations associated with five prominent…

New GSC-II proper motions of RR Lyrae and Blue Horizontal Branch (BHB) stars near the North Galactic Pole are used to show that the Galactic Halo 5 kpc above the Plane has a significantly retrograde galactic rotation.

Astrophysics · Physics 2007-05-23 T. D. Kinman , C. Cacciari , A. Bragaglia , A. Buzzoni , A. Spagna

Three colour photometry on CCD frames in the Special Area SpA23 provides a deep probe of the galactic disc in a low absorption window towards the anticenter. Magnitudes to better than 10% at V = 25 and B-V colour down to V = 23 have been…

Astrophysics · Physics 2011-05-23 Annie C. Robin , Michel Creze , Vijay Mohan

The HESS instrument has observed a diffuse flux of ~ TeV gamma rays from a large solid angle around the Galactic center (GC). This emission is correlated with the distribution of gas in the region suggesting that the gamma rays originate in…

We isolate samples of 733 bright (g < 18) and 437 faint (g > 18) high-Galactic latitude blue horizontal branch stars with photometry and spectroscopy in the Sloan Digital Sky Survey (SDSS). Comparison of independent photometric and…

We present Hubble Space Telescope (HST) observations of the nearby, massive, highly rotating hybrid galaxy UGC~12591, along with observations in UV to FIR bands. HST data in V, I, and H bands is used to disentangle the structural…

We have successfully constructed a catalog of HI-rich galaxies selected from the Minnesota Automated Plate Scanner Catalog of the Palomar Observatory Sky Survey (POSS I) based solely on optical criteria. We identify HI-rich candidates by…

Astrophysics · Physics 2009-11-07 J. E. Cabanela , J. M. Dickey

We report the first results of star counts carried out with the National Astronomical Observatories (NAOC) 60/90 cm Schmidt Telescope in 15 intermediate-band filters from 3000 to 10000 {\AA} in the BATC survey. We analyze a sample of over…

Astrophysics · Physics 2009-11-07 Cuihua Du , Xu Zhou , Jun Ma , Alfred B-C Chen , Yanbin Yang , Jiuli Li , Hong Wu , Zhaoji Jiang , Jiansheng Chen

Red supergiant stars (RSGs) represent the final evolutionary phase of the majority of massive stars and hold a unique role in testing the physics of stellar models. Eighty eight RSGs in the Small Magellanic Cloud (SMC) were recently found…

Solar and Stellar Astrophysics · Physics 2025-08-06 L. R. Patrick , D. J. Lennon , A. Schootemeijer , L. Bianchi , I. Negueruela , N. Langer , D. Thilker , R. Dorda

We present an analysis of the photometric parallaxes of stars in 21 BATC fields carried out with the National Astronomical Observatories (NAOC) 60/90 cm Schmidt Telescope in 15 intermediate-band filters from 3000 to 10000 {\AA}. In this…

Astrophysics · Physics 2009-11-11 Cuihua Du , Jun Ma , Zhenyu Wu , Xu Zhou

A pole-count analysis of the infrared 2MASS survey is presented, in order to identify faint stream-like structures within the halo of the Milky Way. Selecting stars with colours consistent with M-giant stars, we find a strong over-density…

Astrophysics · Physics 2016-08-30 R. A. Ibata , G. F. Lewis , M. J. Irwin , L. Cambresy

The southern Galactic plane has been mapped at optical wavelengths and at under one-arcsecond angular resolution by the VST Photometric Ha Survey of the Galactic plane and bulge (VPHAS+). Anticipating the release of a uniform photometric…

Astrophysics of Galaxies · Physics 2025-12-02 J. E. Drew , R. Greimel , J. Eislöffel , R. Raddi , N. J. Wright

High velocity gas that does not conform to Galactic rotation is observed throughout the Galaxy's halo. One component of this gas, HI high velocity clouds (HVCs), have attracted attention since their discovery in the 1960s and remain…

Astrophysics of Galaxies · Physics 2017-08-24 Asger Grønnow , Thor Tepper-García , Joss Bland-Hawthorn , Naomi McClure-Griffiths

Important tracers for the dark matter halo of the Galaxy are hypervelocity stars (HVSs), which are faster than the local escape velocity of the Galaxy and their slower counterparts, the high-velocity stars in the Galactic halo. Such HVSs…

Solar and Stellar Astrophysics · Physics 2017-05-03 E. Ziegerer , U. Heber , S. Geier , A. Irrgang , T. Kupfer , F. Fürst , J. Schaffenroth

We explore the stellar mass density and colour profiles of 118 low redshift, massive, central galaxies, selected to have assembled 90 percent of their stellar mass 6 Gyr ago, finding evidence of the minor merger activity expected to be the…

Astrophysics of Galaxies · Physics 2023-01-10 Thomas M. Jackson , Anna Pasquali , Francesco La Barbera , Surhud More , Eva K. Grebel

Atmospheric parameters (effective temperature, surface gravity) and radial velocities are derived for 12 candidate blue horizontal branch (HB) stars in the globular clusters 47 Tuc and NGC 362, which so far have been known to contain…

Astrophysics · Physics 2007-05-23 S. Moehler , W. B. Landsman , B. Dorman