Lines of research: The Milky Way and the Local Group (MWLG)
The Milky Way and the Local Group (MWLG)
Grant
Grants Ramón y Cajal: Call 2013
Ramón y Cajal contract to develop his research work in the specific research project "Nucleosynthesis and molecular processes in the last stages of stellar...
Green, solventless debromination of C 70 Br 10 to C 70 with CsI
A smooth, solventless and solid state debromination of C70Br10 can be achieved in a CsI matrix with the restoration of the pristine C70 in quantitative yields...
Ground-based Multisite Observations of Two Transits of HD 80606b
We present ground-based optical observations of the 2009 September and 2010 January transits of HD 80606b. Based on three partial light curves of the 2009...
GTC/CanariCam Mid-IR Imaging of the Fullerene-rich Planetary Nebula IC 418: Searching for the Spatial Distribution of Fullerene-like Molecules
We present seeing-limited narrow-band mid-IR GTC/CanariCam images of the spatially extended fullerene-containing planetary nebula (PN) IC 418. The narrow-band...
H II Regions Within a Compact High Velocity Cloud. A Nearly Starless Dwarf Galaxy?
Within the SECCO survey we identified a candidate stellar counterpart to the Ultra Compact High Velocity Cloud (UCHVC) HVC274.68+74.70-123 that was suggested by...
H α fluxes and extinction distances for planetary nebulae in the IPHAS survey of the northern galactic plane
We report H α filter photometry for 197 Northern hemisphere planetary nebulae (PNe) obtained using imaging data from the IPHAS survey. H α+[N II] fluxes were...
H α morphologies of star clusters: a LEGUS study of H II region evolution time-scales and stochasticity in low-mass clusters
The morphology of H II regions around young star clusters provides insight into the time-scales and physical processes that clear a cluster's natal gas. We...
H-band discovery of additional second-generation stars in the Galactic bulge globular cluster NGC 6522 as observed by APOGEE and Gaia
We present an elemental abundance analysis of high-resolution spectra for five giant stars spatially located within the innermost regions of the bulge globular...
Hayabusa2 extended mission target asteroid 1998 KY<SUB>26</SUB> is smaller and rotating faster than previously known
Understanding the physical characteristics of small Solar System bodies is important not only for refining formation and evolution models but also for space...