Tipo de publicación: Sin árbitro

  • Publicación
    What Are M31 Disk Planetary Nebulae Trying to Tell Us?
    Over the past eight years we have observed optical spectra of planetary nebulae (PNe) in the disk of M31 using DIS on the 3.5-m ARC telescope at Apache Point...
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    What Are the Goals of Popularising Astronomy for Scientists and Society?
    This project addresses the reasons that may motivate efforts to popularize astronomy. Data relevant to this research question were collected by means of focus...
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    What Are We Learning from the Sun?
    Not Available
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    What Can the Radial Surface Brightness Profiles of Galaxy Discs Tell Us About Their Evolution?
    Deriving the azimuthally averaged radial surface brightness profile of a galaxy is a schematic way of presenting the light and then the mass structure of disc...
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    What can we learn from constraining Extreme-Emission Line Galaxies models with large samples of local analogs?
    Extreme Emission Line Galaxies (EELGs) are characterized by their compact sizes and very high equivalent widths of certain optical emission lines (e.g. EW([OIII...
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    What can we learn from near-infrared colours os spiral galaxies?
    Not Available
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    What Can We Learn on the Structure and the Dynamics of the Solar Core with g Modes?
    The detection of the signature of dipole gravity modes has opened the path to study the solar inner radiative zone. Indeed, g modes should be the best probes to...
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    What Disc Brightness Profiles Can Tell us about Galaxy Evolution
    Azimuthally averaged surface brightness profiles of disc galaxies provide a most useful practical classification scheme which gives insights into their...
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    What do Astrophysics and the World's Oldest Profession have in Common?
    In the present paper I want to tell of my impressions about the world of research in astrophysics, which I know from close observation. I see with certain...