Search Results - "Caulet, Adeline"

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    INFRARED SPECTRAL MAPPING OF SUPERNOVA REMNANTS. I. N63A AND ITS ENVIRONMENT by CAULET, Adeline, WILLIAMS, Rosa M

    Published in The Astrophysical journal (20-12-2012)
    “…We present Spitzer Space Telescope spectra of the supernova remnant (SNR) N63A and its native H II region N63 in the Large Magellanic Cloud. We measure nebular…”
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    Journal Article
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    Young Stellar Objects in the Large Magellanic Cloud: N63 and N180 H II Regions by Caulet, Adeline, Gruendl, R. A, Chu, Y.-H

    Published in The Astrophysical journal (01-05-2008)
    “…We used Spitzer infrared observations to find the young stars of two H ii regions in the Large Magellanic Cloud, N63 and N180. The young stellar object (YSO)…”
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    Emission‐Line Properties of the Large Magellanic Cloud Bubble N70 by Skelton, Brooke P., Waller, William H., Gelderman, Richard F., Brown, Larry W., Woodgate, Bruce E., Caulet, Adeline, Schommer, Robert A.

    “…We present a spectrophotometric imaging study of the emission bubble N70 (DEM 301) in the Large Magellanic Cloud. N70 is approximately 100 pc in size with a…”
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    Journal Article
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    Discovery of an M8.5 Dwarf With Proper Motion mu=2.38 arcsec/yr by Lepine, Sebastien, Rich, R. Michael, Neill, James D, Caulet, Adeline, Shara, Michael M

    Published 07-11-2002
    “…Astrophys.J. 581 (2002) L47-L50 We report the discovery of LSR1826+3014, a very faint (V=19.36) star with a very large proper motion (mu=2.38 arcsec/yr). A low…”
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    The First Orbital Period for a Dwarf Nova in a Globular Cluster: V101 in M5 by Neill, James D, Shara, Michael M, Caulet, Adeline, Buckley, David A. H

    Published 08-03-2002
    “…Astron.J.123:3298,2002 We report the first orbital period determination for a Dwarf Nova (DN) in a glubular cluster: V101 in M5 has a period of 5.796 +- 0.036…”
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    Detection of Pre-Shock Dense Circumstellar Material of SN 1978K by Chu, You-Hua, Caulet, Adeline, Montes, Marcos, Panagia, Nino, Van Dyk, Schuyler, Weiler, Kurt

    Published 11-12-1998
    “…The supernova SN 1978K has been noted for its lack of emission lines broader than a few thousand km/s since its discovery in 1990. Modeling of the radio…”
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    Emission-Line Properties of the LMC Bubble N70 by Skelton, Brooke P, Waller, William H, Gelderman, Richard F, Brown, Larry, Woodgate, Bruce, Caulet, Adeline, Schommer, Robert A

    Published 26-02-1999
    “…We present a spectrophotometric imaging study of the emission bubble N70 (DEM 301) in the Large Magellanic Cloud. N70 is approximately 100 pc in size with a…”
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    Journal Article