Results 61 to 70 of about 20,011 (211)
oMEGACat. VII. Tracing Interstellar and Intracluster Medium of ω Centauri Using Sodium Absorptions
We investigate the foreground interstellar medium along the line of sight and intracluster medium of ω Centauri ( ω Cen) by measuring the equivalent width of Na I D absorptions from MUSE observations. The large line-of-sight velocity difference between ω
Z. Wang +16 more
doaj +1 more source
Large Interstellar Polarisation Survey
Our understanding of dust in the diffuse interstellar medium remains incomplete with regard to the structure, composition, size distribution, and alignment properties of its grains.
Siebenmorgen Ralf +4 more
doaj +1 more source
The Panchromatic Hubble Andromeda Treasury. XX. The Disk of M31 is Thick
We present a new approach to measuring the thickness of a partially face-on stellar disk, using dust geometry. In a moderately-inclined disk galaxy, the fraction of reddened stars is expected to be 50% everywhere, assuming that dust lies in a thin ...
Julianne J. Dalcanton +8 more
doaj +1 more source
We present a photometric study of the neglected open cluster Berkeley 53. We derived its fundamental parameters, such as the age, the interstellar reddening, and the distance from the Sun, based on BV photometry combined with near-infrared JHK data.
Dias +12 more
core +2 more sources
Non-uniform extinction in young open star clusters [PDF]
The extinction law and the variation of colour excess with position, luminosity as well as spectral class in young open star clusters NGC 663, NGC869, NGC 884, NGC 1502, NGC 1893, NGC 2244, NGC 2264, NGC 6611, Tr 14, Tr 15,Tr 16, Coll 228, Tr 37 and Be ...
Sagar, Ram, Yadav, R. K. S.
core +3 more sources
The 2000 outburst of the recurrent nova CI Aquilae: optical spectroscopy
We present low- and medium resolution spectra of the recurrent nova CI Aquilae taken at 14 epochs in May and June, 2000. The overall appearance is similar to other U Sco-type recurrent novae (U Sco, V394 CrA).
Anupama +22 more
core +1 more source
Properties of extragalactic dust inferred from linear polarimetry of Type Ia Supernovae [PDF]
Aims: The aim of this paper is twofold: 1) to investigate the properties of extragalactic dust and compare them to what is seen in the Galaxy; 2) to address in an independent way the problem of the anomalous extinction curves reported for reddened Type ...
Baade, D. +11 more
core +3 more sources
Interstellar Reddening Effect on the Age Dating of Population II Stars
The age measurement of the stellar halo component of the Galaxy is based mainly on the comparison of the main sequence turn-off luminosity of the globular cluster (GC) stars with theoretical isochrones.
Sergio Ortolani +2 more
doaj +1 more source
The Effect of a Nonuniversal Extinction Curve on the Wesenheit Function and Cepheid Distances
The Wesenheit function is widely used to reduce the effects of interstellar reddening in distance measurements. Its construction, however, relies on the assumption of a universal extinction curve and on fixed values of the total-to-selective extinction ...
Dorota M. Skowron +3 more
doaj +1 more source
Three-dimensional Reddening Maps of the Magellanic Clouds Constructed by RR Lyrae Stars
We present the first three-dimensional reddening maps of the Large and Small Magellanic Clouds (LMC and SMC) constructed using fundamental-mode RR Lyrae stars (RRab) from the Optical Gravitational Lensing Experiment (OGLE) survey.
Shun-Xuan He, Yang Huang
doaj +1 more source

