We present the discovery of an inhomogenous, low-surface brightness, extended disk-like structure around the Andromeda galaxy (M31) based on a large kinematic survey of more than 2800 stars with the Keck/DEIMOS multi-object spectrograph. The stellar structure spans radii from 15 kpc out to ∼ 40 kpc, with detections out to R ∼ 70 kpc. The constituent stars lag the expected velocity of circular o...

Background: One of the acute hematologic malignancies is acute promyelocytic leukemia (APL) that resulted in translocation of chromosomes 15 and 17, t (15; 17), and cessation in the maturation of myeloid cell line, and ultimate aggregation of neoplastic promyelocytes. Regarding that appetence of using herbal and marine medicine studies is increasing, and on the other hand, the features of Cassi...

We present a new deep 21-cm survey of the Andromeda galaxy, based on high resolution observations performed with the Synthesis Telescope and the 26-m antenna at DRAO. The Hi distribution and kinematics of the disc are analyzed and basic dynamical properties are given. The rotation curve is measured out to 38 kpc, showing a nuclear peak at 340 km s, a dip at 202 km s around 4 kpc, two distinct f...

The global missing baryon problem — that the sum of observed baryons falls short of the number expected form BBN — is well known. In addition to this, there is also a local missing baryon problem that applies to individual dark matter halos. This halo by halo missing baryon problem is such that the observed mass fraction of baryons in individual galaxies falls short of the cosmic baryon fractio...

Andromeda is a wideeld, imaging, hard X-ray/soft gamma-ray instrument capable of detecting gamma-ray bursts (GRBs) a factor 20 times fainter than GRO/BATSE. During 1-year of a two-year mission, it could determine whether GRBs are Galactic or cosmological in origin by searching for an excess of bursts towards the nearby Andromeda galaxy (M31). As a pointed, imaging instrument with sensitivity in...

Abstract This Letter develops a method to constrain the cosmological constant Λ from binary galaxies, focusing on Milky Way and Andromeda galaxies. We provide an analytical solution two-body problem with show that ratio between Keplerian period <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" ove...