Spectral observations of the systems with the disturbed spiral arms: Arp 42, Arp 82, and Arp 58
نویسندگان
چکیده
منابع مشابه
Continuum and spectral line observations of the OH Megamaser galaxy Arp 220
We present MERLIN observations of the continuum (both 1.6 and 5 GHz) and OH maser emission towards Arp 220. The correct spatial configuration of the various components of the galaxy is revealed. In the eastern component the masers are shown to be generally coincident with the larger-scale continuum emission; in the west, the masers and continuum do not generally arise from the same location. A ...
متن کاملArp bent out of shape
iochemical and kinetic studies have failed to provide a unified view on how the Arp2/3 complex nucleates actin filaments. Does the complex, which mediates actin filament nucleation and branch formation at the leading edge of motile cells, bind to the side of an older actin filament, or does it become incorporated into that filament? B Structural studies now add a new dimension to the discourse,...
متن کاملARP/wARP and molecular replacement.
The aim of ARP/wARP is improved automation of model building and refinement in macromolecular crystallography. Once a molecular-replacement solution has been obtained, it is often tedious to refine and rebuild the initial (search) model. ARP/wARP offers three options to automate that task to varying extents: (i) autobuilding of a completely new model based on phases calculated from the molecula...
متن کاملAtomic carbon in Arp 220
We present detections of the 3 P 1 ? 3 P 0 ne-structure line of neutral carbon, and of the J = 3 ? 2 rotational line of carbon monoxide in the ultraluminous infrared galaxy Arp 220, obtained at the Caltech Submillimeter Observatory. C I emission in Arp 220 is found to be at the expected level in relation to the strong FIR dust emission and to the CO emission, whereas the C II emission seen by I...
متن کاملH I and CO observations of Arp 104 : a spiral – elliptical interacting pair
We present data probing the spatial and kinematical distribution of both the atomic (H I) and molecular (CO) gas in NGC 5218, the late-type barred spiral galaxy in the spiral–elliptical interacting pair, Arp 104. We consider these data in conjunction with far-infrared and radiocontinuum data, and N-body simulations, to study the galaxies interactions, and the star formation properties of NGC 52...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 2019
ISSN: 0035-8711,1365-2966
DOI: 10.1093/mnras/stz1025