Results 1 to 10 of about 475 (99)
THE H I CONTENT OF LOCAL LATE-TYPE GALAXIES [PDF]
The Astrophysical Journal, 2011 We present a solid relationship between the neutral hydrogen (HI) disk mass and the stellar disk mass of late-type galaxies in the local universe. This relationship is derived by comparing the stellar disk mass function from the Sloan Digital Sky Survey and the HI mass function from the HI Parkes All Sky Survey (HIPASS).
Evoli, C. +3 more
openaire +3 more sources
Colour-magnitude relations of late-type galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 2006 We use a large sample of galaxies drawn from the Sloan Digital Sky Survey (SDSS) and Two Micro All Sky Survey (2MASS) to present Color-Magnitude Relations (CMRs) for late-type galaxies in both optical and optical-infrared bands. A sample from SDSS Data Release 4 (DR4) is selected to investigate the optical properties.
Chang, Ruixiang +4 more
openaire +2 more sources
CHARACTERISTICS OF SPIRAL ARMS IN LATE-TYPE GALAXIES [PDF]
The Astrophysical Journal, 2015 We have measured the positions of large numbers of H II regions in four nearly face-on, late-type, spiral galaxies: NGC 628 (M 74), NGC 1232, NGC 3184 and NGC 5194 (M 51). Fitting log-periodic spiral models to segments of each arm yields local estimates of spiral pitch angle and arm width.
Honig, Z. N., Reid, M. J.
openaire +2 more sources
Environmental Effects on Late‐Type Galaxies in Nearby Clusters [PDF]
Publications of the Astronomical Society of the Pacific, 2006 Review paper accepted for publication on PASP, high resolution version of the figures available on the GOLDMine webpage: http://goldmine.mib.infn.it/papers ...
Boselli, A., Gavazzi, G.
openaire +4 more sources
Cold Dust in Late‐Type Virgo Cluster Galaxies [PDF]
The Astrophysical Journal, 2002 We have statistically analyzed the spatially integrated far-infrared (FIR) emissions of the complete volume- and luminosity-limited sample of late-type (later than S0) Virgo cluster galaxies measured using the Infrared Space Observatory (ISO) by Tuffs et al. (2002) in bands centered on 60, 100 and 170 microns.
Popescu, C. +4 more
openaire +3 more sources
Stellar Populations in the Nuclei of Late‐Type Spiral Galaxies [PDF]
The Astrophysical Journal, 2006 ApJ submitted (original submission Oct 19, 2005, present version includes changes based on referee recommendations).
Walcher, C. J. +7 more
openaire +4 more sources
[Cii] emission and star formation in late-type galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 1999 A linear correlation between the ratio of the[CII( $$^{\text{2}}$$ P $$_{3/2}$$ →
Pierini, D. +3 more
openaire +2 more sources
Evolution of the spin of late-type galaxies caused by galaxy-galaxy interactions
, 2021 17 pages, 17 figures, 2 tables.
Hwang, Jeong-Sun +3 more
openaire +2 more sources
Magnetic fields in late-type galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 1993 Magnitudes of the volume-averaged magnetic field have been derived for a representative sample of 146 late-type galaxies using the minimum-energy condition and a simple model for the distribution of radio-emitting plasma within these galaxies. The distribution of derived magnetic fields is narrow (B eq = 0.29 ± 0.11 nT) and skewed to higher values ...
A. J. Fitt, P. Alexander
openaire +1 more source
Angular momenta of late-type spiral galaxies [PDF]
Symposium - International Astronomical Union, 1970 The angular momenta of galaxies may be evaluated from their photometry. The mass to light ratio in NGC 224 is discussed and the calculation is applied to two late-type spirals.
openaire +1 more source