DOCSLIB.ORG
Explore
Sign Up
Log In
Upload
Search
Home
» Tags
» Maia (star)
Maia (star)
Hot Interstellar Matter in Elliptical Galaxies
THE 1000 BRIGHTEST HIPASS GALAXIES: H I PROPERTIES B
Winter Constellations
Arxiv:2009.04090V2 [Astro-Ph.GA] 14 Sep 2020
The Formation and Evolution of S0 Galaxies
Download This Article in PDF Format
Globular Clusters and Galactic Nuclei
A Wide-Field H I Study of the NGC 1566 Group*
A Six-Parameter Space to Describe Galaxy Diversification⋆
DEBRIS DISKS in OPEN STELLAR CLUSTERS by Nadiya Igorivna
Prevalence of Tidal Interactions Among Local Seyfert Galaxies
Arxiv:Astro-Ph/0610934V1 31 Oct 2006
Charles Messier (1730-1817) Was an Observational Astronomer Working
2013 Annual Progress Report and 2014 Program Plan of the Gemini Observatory
Description of Pictures in the Dome
Biographical Sketch
Arxiv:1211.6808V1 [Astro-Ph.GA] 29 Nov 2012 Fe R6mdl.Tescn Ehdas Tlzsgas (Here- Utilizes Densities Also a Method Volume Turn Second of Gas the in and Function Model)
Durham Research Online
Top View
ROSAT PSPC and HRI Observations of the Composite Starburst/Seyfert 2 Galaxy NGC 1672 N96-13428
On Possible Explanations of Pulsations in Maia Stars
The Rising Stellar Velocity Dispersion of M87 from Integrated Starlight 3 in Duration and Bracketed by 10 Minute Sky Nods
ALABAMA University Libraries
Annual Report Rapport Annuel Jahresbericht 1997
STEP Survey – II. Structural Analysis of 170 Star Clusters in the SMC
Space Math II
Annual Report Publications 2012
The ANU Wifes Supernova Programme (AWSNAP)
2018 ANNUAL PROGRESS REPORT of the GEMINI OBSERVATORY Table of Contents
II. Observational Constraints on the Progenitors of Type Ibc Supernovae
The SLUGGS Survey: Exploring the Metallicity Gradients of Nearby Early-Type Galaxies to Large Radii
The Tully–Fisher Relation for S0 Galaxies
Stellar Population and the Origin of Intra-Cluster Stars Around Brightest Cluster Galaxies: the Case of NGC 3311
The I-Band Tully-Fisher Relation for Sc Galaxies: 21 Centimeter H I Line Data
A 3-D TOUR of OUR GALAXY Pleiades Praesepe Arcturus
The Angular-Momentum Distribution in Axisymmetrical Galaxies B
The Gaia-ESO Survey: a New Approach to Chemically Characterising Young Open Clusters? II