Sandage, Becklin, and Neugebauer (1969) have confirmed and extended the color aperture relation for M 31 over the region within T from the nucleus first reported by de Vaucouleurs and Tifft (de Vaucouleurs 1961). In view of the importance of the spectral energy distribution of M31 in determining the K correction, and also the possible variation of stellar content with distance from the nucleus, we have extended these measurements to larger apertures
Aims. We continue the analysis of the data set of our spectroscopic observation campaign of M 31, wh...
The galaxy M100 = NGC 4321 is a spiral galaxy in which a bright Type II Supernova was discovered on ...
International audienceThe study of extragalactic planetary nebulae (PNe) in the optical regions of g...
New broad-band infrared JHK data and narrow-band CO and H_2O indices for the semistellar nucleus of ...
For a number of places in the bulge of M31 and for two places in M32 photometric scans from 3300 A t...
We have derived the luminosity function for stars in the bulge of M31 in a region ∼7.2′ (1.44 kpc) f...
Observations are presented of equivalent widths for strong spectral features with λ > 5000 Å in the ...
Abstract. We present the results of a study based on an XMM-Newton Performance Verification observat...
A technique is described for obtaining high-sensitivity measurements with high spatial resolution at...
International audienceWe analyze the stellar populations present in M31 by using nine sets of adjace...
Journal ArticleWe present the AGAPE astrometric and photometric catalogue of 1579 variable stars in ...
We present the data and initial results from a combined HST/IUE/ground-based spectroscopic monitorin...
We confirm our earlier tentative detection of M31* in X-rays and measure its light curve and spectru...
We present a study of Hubble Space Telescope Wide Field Planetary Camera 2 observations of the inner...
Data obtained in the 1950-1955 Palomar campaign for the discovery of classical novae in M81 are set ...
Aims. We continue the analysis of the data set of our spectroscopic observation campaign of M 31, wh...
The galaxy M100 = NGC 4321 is a spiral galaxy in which a bright Type II Supernova was discovered on ...
International audienceThe study of extragalactic planetary nebulae (PNe) in the optical regions of g...
New broad-band infrared JHK data and narrow-band CO and H_2O indices for the semistellar nucleus of ...
For a number of places in the bulge of M31 and for two places in M32 photometric scans from 3300 A t...
We have derived the luminosity function for stars in the bulge of M31 in a region ∼7.2′ (1.44 kpc) f...
Observations are presented of equivalent widths for strong spectral features with λ > 5000 Å in the ...
Abstract. We present the results of a study based on an XMM-Newton Performance Verification observat...
A technique is described for obtaining high-sensitivity measurements with high spatial resolution at...
International audienceWe analyze the stellar populations present in M31 by using nine sets of adjace...
Journal ArticleWe present the AGAPE astrometric and photometric catalogue of 1579 variable stars in ...
We present the data and initial results from a combined HST/IUE/ground-based spectroscopic monitorin...
We confirm our earlier tentative detection of M31* in X-rays and measure its light curve and spectru...
We present a study of Hubble Space Telescope Wide Field Planetary Camera 2 observations of the inner...
Data obtained in the 1950-1955 Palomar campaign for the discovery of classical novae in M81 are set ...
Aims. We continue the analysis of the data set of our spectroscopic observation campaign of M 31, wh...
The galaxy M100 = NGC 4321 is a spiral galaxy in which a bright Type II Supernova was discovered on ...
International audienceThe study of extragalactic planetary nebulae (PNe) in the optical regions of g...