TYPE II SUPERNOVAE AS DISTANCE INDICATORS by Mario
... Enrico Capallaro, and Massimo Turatto, for allowing me to use their spectra and photometry obtained in the course of the ESO Supernova Key Project, and from Mark Phillips and Sofia Kirhakos for making available their extensive dataset of SN 1986L. A special thank must go to Ron Eastman for providing ...
... Enrico Capallaro, and Massimo Turatto, for allowing me to use their spectra and photometry obtained in the course of the ESO Supernova Key Project, and from Mark Phillips and Sofia Kirhakos for making available their extensive dataset of SN 1986L. A special thank must go to Ron Eastman for providing ...
https://tel.archives-ouvertes.fr/file/index/docid/1058049/filename/HOU_XIAN_2013.pdf
... be a graduate student working on Fermi gamma-ray pulsars in the Astroparticle group in CENBG, and for having accompanied me in these three years with his fruitful instructive guidance in my work. I appreciate also his American humor and his optimistic attitude for the life, which have brought me hap ...
... be a graduate student working on Fermi gamma-ray pulsars in the Astroparticle group in CENBG, and for having accompanied me in these three years with his fruitful instructive guidance in my work. I appreciate also his American humor and his optimistic attitude for the life, which have brought me hap ...
Trans-Neptunian objects as natural probes to the unknown solar
... Trans-Neptunian objects (TNOs) are icy/rocky bodies that move beyond the orbit of Neptune in a region known as the trans-Neptunian belt (or Edgeworth-Kuiper belt). TNOs are believed to be the remnants of a collisionally, dynamically and chemically evolved protoplanetary disk composed of billions of ...
... Trans-Neptunian objects (TNOs) are icy/rocky bodies that move beyond the orbit of Neptune in a region known as the trans-Neptunian belt (or Edgeworth-Kuiper belt). TNOs are believed to be the remnants of a collisionally, dynamically and chemically evolved protoplanetary disk composed of billions of ...
Binary and Millisecond Pulsars | SpringerLink
... members of eclipsing binary systems which could hamper their detection in radio surveys. Independent constraints on the limiting spin frequencies of neutron stars come from studies of millisecond X-ray binaries [66] which are not thought to be selection-effect limited [67]. This analysis does not pr ...
... members of eclipsing binary systems which could hamper their detection in radio surveys. Independent constraints on the limiting spin frequencies of neutron stars come from studies of millisecond X-ray binaries [66] which are not thought to be selection-effect limited [67]. This analysis does not pr ...
Discovery and Study of Exotic Radio Pulsars Jason William Thomas
... the Arecibo telescope. It is the deepest search of these clusters ever conducted. Our survey employed a higher observing frequency and higher resolution datarecording than the only previous major survey of these clusters with Arecibo, which was conducted 10 years prior to the start of our survey. We ...
... the Arecibo telescope. It is the deepest search of these clusters ever conducted. Our survey employed a higher observing frequency and higher resolution datarecording than the only previous major survey of these clusters with Arecibo, which was conducted 10 years prior to the start of our survey. We ...
Advanced LIGO—the Next Generation
... » International support and significant material participation » Especially strong collaboration with German-UK GEO group, capital partnership Advanced LIGO design, R&D, and fabrication shared with ...
... » International support and significant material participation » Especially strong collaboration with German-UK GEO group, capital partnership Advanced LIGO design, R&D, and fabrication shared with ...
HUBBLE SPACE TELESCOPE AND GROUND-BASED
... of SNe Iax, Lyman et al. (2013) find a statistical association with star forming regions similar to that of SNe IIP. The two objects we focus on in this work, SN 2005hk and SN 2008A, are both in star-forming galaxies, but there is no evidence for star formation at the location of either object (Lyma ...
... of SNe Iax, Lyman et al. (2013) find a statistical association with star forming regions similar to that of SNe IIP. The two objects we focus on in this work, SN 2005hk and SN 2008A, are both in star-forming galaxies, but there is no evidence for star formation at the location of either object (Lyma ...
- REAL-J
... 4625 V. KESKIN, Z. ASLAN: First Photometric Observations at the Turkish National Observatory : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : 1 { 2 4626 L.N. BERDNIKOV, D.G. TURNER: Observations of II Carinae, a 65-day Classical Cepheid ...
... 4625 V. KESKIN, Z. ASLAN: First Photometric Observations at the Turkish National Observatory : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : 1 { 2 4626 L.N. BERDNIKOV, D.G. TURNER: Observations of II Carinae, a 65-day Classical Cepheid ...
Slides - AO4ELT3
... reflected light will tell us how many planetary systems actually share the same “architecture” as our own ...
... reflected light will tell us how many planetary systems actually share the same “architecture” as our own ...
H i AND CO IN BLUE COMPACT DWARF GALAXIES: HARO 2 AND
... led many BCDs to be classified as H ii galaxies (although, in general, not all H ii galaxies are necessary dwarf systems). At their current star formation rates (SFRs), these systems would exhaust their total available gas in considerably less than a Hubble time; for this reason, it is generally acc ...
... led many BCDs to be classified as H ii galaxies (although, in general, not all H ii galaxies are necessary dwarf systems). At their current star formation rates (SFRs), these systems would exhaust their total available gas in considerably less than a Hubble time; for this reason, it is generally acc ...
Lyman-alpha imaging of starburst galaxies in the local universe and beyond Matthew Hayes
... The universe is a large and poorly understood entity. A great deal of what we do understand comes from observations of the stars; by observing the radiation they produce directly, by observing reprocessed stellar energy, or by observing the violent phenomena in the final stages of stellar evolution. ...
... The universe is a large and poorly understood entity. A great deal of what we do understand comes from observations of the stars; by observing the radiation they produce directly, by observing reprocessed stellar energy, or by observing the violent phenomena in the final stages of stellar evolution. ...
From Filamentary Networks to Dense Cores in Molecular Clouds
... 2.1 Evidence of interstellar filaments prior to Herschel The presence of parsec-scale filamentary structures in nearby interstellar clouds and their potential importance for star formation have been pointed out by many authors for more than three decades. For example, Schneider and Elmegreen (1979) ...
... 2.1 Evidence of interstellar filaments prior to Herschel The presence of parsec-scale filamentary structures in nearby interstellar clouds and their potential importance for star formation have been pointed out by many authors for more than three decades. For example, Schneider and Elmegreen (1979) ...
Galaxy Formation and Evolution.
... This publication is in copyright. Subject to statutory exception and to the provision of relevant collective licensing agreements, no reproduction of any part may take place without the written permission of Cambridge University Press. ...
... This publication is in copyright. Subject to statutory exception and to the provision of relevant collective licensing agreements, no reproduction of any part may take place without the written permission of Cambridge University Press. ...
