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S.D. Doty

Identifiers

  • name variant S.D. Doty 0.60 · backfill

Papers (19)

  1. Water in star-forming regions with Herschel (WISH): II. Evolution of 557 GHz 110-101 emission in low-mass protostars astro-ph.SR · 2012 · author #15
  2. HERSCHEL-HIFI spectroscopy of the intermediate mass protostar NGC7129 FIRS 2 astro-ph.SR · 2010 · author #28
  3. Herschel-HIFI observations of high-J CO lines in the NGC 1333 low-mass star-forming region astro-ph.SR · 2010 · author #9
  4. Variations in H2O+/H2O ratios toward massive star-forming regions astro-ph.GA · 2010 · author #29
  5. Water in massive star-forming regions: HIFI observations of W3 IRS5 astro-ph.SR · 2010 · author #27
  6. Herschel-HIFI detections of hydrides towards AFGL 2591 (Envelope emission versus tenuous cloud absorption) astro-ph.SR · 2010 · author #5
  7. Water in low-mass star-forming regions with Herschel: HIFI spectroscopy of NGC1333 astro-ph.SR · 2010 · author #5
  8. Sensitive limits on the abundance of cold water vapor in the DM Tau protoplanetary disk astro-ph.SR · 2010 · author #29
  9. Water vapor toward starless cores: the Herschel view astro-ph.GA · 2010 · author #25
  10. Herschel-PACS spectroscopy of the intermediate mass protostar NGC7129 FIRS 2 astro-ph.GA · 2010 · author #35
  11. Origin of the hot gas in low-mass protostars: Herschel-PACS spectroscopy of HH 46 astro-ph.SR · 2010 · author #9
  12. The chemical history of molecules in circumstellar disks. I. Ices astro-ph.SR · 2009 · author #3
  13. Infrared Molecular Starburst Fingerprints in Deeply Obscured (U)LIRG Nuclei astro-ph · 2006 · author #4
  14. Tracing high energy radiation with molecular lines near deeply embedded protostars astro-ph · 2006 · author #5
  15. Water destruction by X-rays in young stellar objects astro-ph · 2006 · author #4
  16. X-ray chemistry in envelopes around young stellar objects astro-ph · 2005 · author #2
  17. X-ray Chemistry in the Envelopes around Young Stellar Objects astro-ph · 2004 · author #3
  18. Influence of UV radiation from a massive YSO on the chemistry of its envelope astro-ph · 2004 · author #2
  19. Numerical methods for non-LTE line radiative transfer: Performance and convergence characteristics astro-ph · 2002 · author #5

Mentions

  • 1204.0009 #15 · backfill · confidence 0.70 S.D. Doty
  • 1008.1254 #28 · backfill · confidence 0.70 S.D. Doty
  • 1008.0867 #9 · backfill · confidence 0.70 S.D. Doty
  • 1007.4370 #29 · backfill · confidence 0.70 S.D. Doty
  • 1007.3986 #27 · backfill · confidence 0.70 S.D. Doty
  • 1007.3408 #5 · backfill · confidence 0.70 S.D. Doty
  • 1007.3031 #5 · backfill · confidence 0.70 S.D. Doty
  • 1007.2129 #29 · backfill · confidence 0.70 S.D. Doty
  • 1007.1248 #25 · backfill · confidence 0.70 S.D. Doty
  • 1006.0210 #35 · backfill · confidence 0.70 S.D. Doty
  • 1005.2031 #9 · backfill · confidence 0.70 S.D. Doty
  • 0901.1313 #3 · backfill · confidence 0.70 S.D. Doty

Frequent Coauthors