The parameter multiple takes the value M if the object belongs to a multiple system. For example, a galaxy belonging to a pair of galaxies have multiple=M . Presently multiple accounts for the association in projection on the sky and therefore does not reflect for sure a physical association: members of "false" pairs will have multiple=M . ... The simple membership to a cluster of galaxies does not imply a galaxy to carry multiple=M . ... HyperLeda . ...

It is now possible to specify multiple log files, each with a fully customizable format. ... Multiple log files are implemented as part of the mod_log_config module which as of Apache 1.2 is the default log module. Multiple log files be created with either the TransferLog or CustomLog directive. These directives can be repeated to create more than one log file (in previous releases, only one logfile could be given per server configuration). ... Syntax: CustomLog filename "format" . ...

... Both selfcal and gpscal can be given multiple input model images. ... The self-calibration tasks assume that the gains are not dependent on these different aspects of the data ( e.g. the gains are independent of frequency and pointing centre). ... The self-calibration tasks will generally determine the appropriate correspondence between data and model ( e.g. it will associate the data from a particular pointing with a model with the same pointing). ...

... Recent studies indicate that stars are most likely forming within the binary and multiple systems. ... During several years we are conducting the observations of such multiple stellar systems at the BTA telescope in order to find their companions and study the properties therein. ... This star is interesting in that it may be a dynamically unstable multiple star, meaning that over time, such systems will split into individual stars. ... A bright component is a very tight spectroscopic binary star. ...

... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: Dynamical models of multiple globular cluster populations around massive galaxies . ... Different techniques have been devised to separate multiple GC populations and perform dynamical analyses. ... Within this project, the PhD candidate will examine mock models of multiple GC populations around massive galaxies, devising `blinded' functional tests and comparing the possible sources of bias in different techniques....

Chapter 15. Configuring Multiple X Screens on One Card . ... GPUs that support TwinView ( Chapter 13, Configuring TwinView ) can also be configured to treat each connected display device as a separate X screen. ... X has historically used one screen per display device. To configure two separate X screens to share one graphics card, here is what you will need to do: . ... Screen 0 "Screen0" Screen 1 "Screen1" leftOf "Screen0" .. ... Configuring GLX in Xinerama . ... Configuring TV-Out ...

... The necessity of simultaneous access to one communication channel by many users, e.g., in satellite communication systems or cellular telephony, has led to the development of the corresponding standards: FDMA (Frequency Division Multiple Access) and TDMA (Frequency Division Multiple Access). ... There is a number of ideas for chaotic signal applications in multiple-access systems, but as a rule, chaotic signals are used there only as efficient and versatile means of quasi-noise signal formation. ...

. To print multiple copies of a file use the # (hash) option. For example: lpr -#3 memo.txt . This prints three copies of the file memo.txt on your default printer. You can also print multiple copies of several files. For example: lpr -Pps1 -#3 survey.doc letter.txt . This prints three copies of the files survey.doc and letter.txt on the printer ps1 . Tip ...

We present and discuss the results of new multiple-scattering radiative transfer calculations for three representative types of galactic environments, filled with either homogeneous or two-phase clumpy dust distributions. ... The examination of the models concentrates on the study of UV/visual/near-IR reddening effects, the wavelength dependence of attenuation, and on the changes that arise from the transition from homogeneous to clumpy dust distributions in different star/dust geometries. ...