Results 231 to 240 of about 176,382 (265)

Primordial Rotating Disk Composed of ≥15 Star Forming Clumps at Cosmic Dawn

Fujimoto S, Ouchi M, Kohno K, Valentino F, Giménez-Arteaga C, Brammer G, Furtak L, Kohandel M, Oguri M, Pallottini A, Richard J, Zitrin A, Bauer F, Boylan-Kolchin M, Dessauges-Zavadsky M, Egami E, Finkelstein S, Ma Z, Smail I, Watson D, Hutchison T, Rigby J, Welch B, Ao Y, Bradley L, Caminha G, Caputi K, Espada D, Endsley R, Fudamoto Y, González-López J, Hatsukade B, Koekemoer A, Kokorev V, Laporte N, Lee M, Magdis G, Ono Y, Rizzo F, Shibuya T, Shimasaku K, Sun F, Toft S, Umehata H, Wang T, Yajima H.   +45 more
europepmc   +1 more source

Magellanic Clouds: VIII. On the Population Characteristics of the Two Clouds. [PDF]

Proc Natl Acad Sci U S A, 1953
Shapley H.
europepmc   +1 more source

Magellanic Clouds: IV. On the Period Frequency Anomalies. [PDF]

Proc Natl Acad Sci U S A, 1952
Shapley H, Nail VM.
europepmc   +1 more source

Galactic and Extragalactic Studies: IV. Photometry of Two Large Southern Clusters of Galaxies. [PDF]

Proc Natl Acad Sci U S A, 1940
Shapley H, Boyd CD.
europepmc   +1 more source

Galactic and Extragalactic Studies: XVII. Revision of the Distances of Thirty High-Latitude Globular Clusters. [PDF]

Proc Natl Acad Sci U S A, 1944
Shapley H.
europepmc   +1 more source

Galactic and Extragalactic Studies: II. Notes on the Peculiar Stellar Systems in Sculptor and Fornax. [PDF]

Proc Natl Acad Sci U S A, 1939
Shapley H.
europepmc   +1 more source

Summary of Investigations of Variable Stars. [PDF]

Proc Natl Acad Sci U S A, 1936
Shapley H.
europepmc   +1 more source

Structure-dynamics relations for late-type spiral and dwarf irregular galaxies revisited

, 2018
Bernhard R. Parodi
openalex   +2 more sources

Some of the next articles are maybe not open access.

Related searches:

A constant intrinsic thickness for dwarf irregular galaxies?

Monthly Notices of the Royal Astronomical Society: Letters, 2016
Abstract We assess the intrinsic thickness parameter, qo, for a sample of dwarf irregular galaxies and compare to larger, more massive spiral galaxy systems. We use optical photometry to determine b/a (minor-to-major axial ratio), and we use the H i kinematic inclination angle to derive qo.
M. Johnson, Peter Kamphuis, Jing Wang, Deidre A. Hunter   +3 more
openaire   +3 more sources

Dwarf Irregular Galaxies of the Local Group

2014
Local Group dwarf irregulars (dIrrs) cover an enormous range in star formation properties. Here I discuss these tiny galaxies as probes of star formation at the extremes of low gas densities and low metallicities. We have learned that (1) Star formation is inefficient in dIrrs and yet at very low \(\Sigma_{\rm HI}\) (\(
D. Hunter
openaire   +3 more sources