Physical and Kinematical Properties of NGC 4214
Not Available
Maiz-Apellaniz, J. et al.
Advertised on:
5
1997
This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..
It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/
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Old Populations and the Star Formation History of the Local Group Dwarf Irregular Galaxy NGC 6822A method for studying the full star formation history (SFH) of nearby galaxies,as a function of time, has been developped and implemented. For the first time, the full SFH of a nearby dwarf irregular galaxy (DIG) has been retrieved from the photometry of its resolved stars. NGC~6822 has been observed in $UBVRI$ at the 2.5m INT telescope, at theGallart, C.
Advertised on:
51997 -
Old Populations and the Star Formation History of the Local Group Dwarf Irregular Galaxy NGC 6822A method for studying the star formation history (SFH) of nearby galaxies, as a function of time, has been developped and implemented. For the first time, the full SFH of a nearby dwarf irregular galaxy (DIG) has been retrieved from the photometry of its resolved stars. In the [(V-I),I] colour-magnitude diagram (CMD) of about 18000 stars in NGCGallart, C. et al.
Advertised on:
51997 -
Observations of Doppler oscillations in a solar prominenceNot AvailableBaudin, F. et al.
Advertised on:
51997 -
New Cosmological Structures on Medium Angular Scales Detected with the Tenerife ExperimentsWe present observations at 10 and 15 GHz taken with the Tenerife experiments in a band of the sky at declination +35 deg. These experiments are sensitive to multipoles in the range l = 10--30. The sensitivities per beam are 56 and 20 mu K for the 10 and 15 GHz data, respectively. After subtraction of the prediction of known radio sources, theGutierrez, C. M. et al.
Advertised on:
51997 -
Multiwavelength observations of the February 1996 high-energy flare in the blazar 3C 279We report CGRO, RXTE, ASCA, ROSAT, IUE, HST and ground-based observations of a large flare in 3C 279 in February 1996. X-rays and γ-rays peaked simultaneously (within one day). We show simultaneous spectral energy distributions prior to and near the flare peak. The γ-ray flare was the brightest ever observed in this source.Wehrle, A. E. et al.
Advertised on:
51997