THE ionized circumstellar envelopes of orion source i and the becklin-neugebauer object

R. L. Plambeck, A. D. Bolatto, J. M. Carpenter, Joshua A Eisner, J. W. Lamb, E. M. Leitch, Daniel P Marrone, S. J. Muchovej, L. M. Pérez, M. W. Pound, P. J. Teuben, N. H. Volgenau, D. P. Woody, M. C H Wright, B. A. Zauderer

Research output: Contribution to journalArticle

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Abstract

The 229 GHz (λ1.3 mm) radio emission from Orion-KL was mapped with up to 0.″14 angular resolution with CARMA, allowing measurements of the flux densities of Source I ("SrcI") and the Becklin-Neugebauer Object (BN), the two most massive stars in this region. We find integrated flux densities of 310 ± 45 mJy for SrcI and 240 ± 35 mJy for BN. SrcI is optically thick even at 229 GHz. No trace of the H30α recombination line is seen in its spectrum, although the v 2 = 1, 5(5,0)-6(4,3) transition of H2O, 3450 K above the ground state, is prominent. SrcI is elongated at position angle 140°, as in 43 GHz images. These results are most easily reconciled with models in which the radio emission from SrcI arises via the H- free-free opacity in a T < 4500 K disk, as considered by Reid et al. By contrast, the radio spectrum of BN is consistent with p +/e - free-free emission from a dense (ne ∼ 5 × 107 cm-3), but otherwise conventional, hypercompact H II region. The source is becoming optically thin at 229 GHz, and the H30α recombination line, at V LSR = 23.2 ± 0.5 km s-1, is prominent in its spectrum. A Lyman continuum flux of 5 × 1045 photons s-1, consistent with that expected from a B star, is required to maintain the ionization. Supplementary 90 GHz observations were made to measure the H41α and H42α recombination lines toward BN. Published 43 and 86 GHz data suggest that SrcI brightened with respect to BN over the 15 year period from 1994 to 2009.

Original languageEnglish (US)
Article number40
JournalAstrophysical Journal
Volume765
Issue number1
DOIs
StatePublished - Mar 1 2013

Fingerprint

radio emission
recombination
envelopes
flux density
radio
radio spectra
B stars
H II regions
opacity
angular resolution
massive stars
continuums
ionization
ground state
photons

Keywords

  • ISM: individual objects (Orion-KL)
  • radio continuum: stars
  • radio lines: stars
  • stars: formation
  • stars: individual (Becklin-Neugebauer-Object)

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Plambeck, R. L., Bolatto, A. D., Carpenter, J. M., Eisner, J. A., Lamb, J. W., Leitch, E. M., ... Zauderer, B. A. (2013). THE ionized circumstellar envelopes of orion source i and the becklin-neugebauer object. Astrophysical Journal, 765(1), [40]. https://doi.org/10.1088/0004-637X/765/1/40

THE ionized circumstellar envelopes of orion source i and the becklin-neugebauer object. / Plambeck, R. L.; Bolatto, A. D.; Carpenter, J. M.; Eisner, Joshua A; Lamb, J. W.; Leitch, E. M.; Marrone, Daniel P; Muchovej, S. J.; Pérez, L. M.; Pound, M. W.; Teuben, P. J.; Volgenau, N. H.; Woody, D. P.; Wright, M. C H; Zauderer, B. A.

In: Astrophysical Journal, Vol. 765, No. 1, 40, 01.03.2013.

Research output: Contribution to journalArticle

Plambeck, RL, Bolatto, AD, Carpenter, JM, Eisner, JA, Lamb, JW, Leitch, EM, Marrone, DP, Muchovej, SJ, Pérez, LM, Pound, MW, Teuben, PJ, Volgenau, NH, Woody, DP, Wright, MCH & Zauderer, BA 2013, 'THE ionized circumstellar envelopes of orion source i and the becklin-neugebauer object', Astrophysical Journal, vol. 765, no. 1, 40. https://doi.org/10.1088/0004-637X/765/1/40
Plambeck, R. L. ; Bolatto, A. D. ; Carpenter, J. M. ; Eisner, Joshua A ; Lamb, J. W. ; Leitch, E. M. ; Marrone, Daniel P ; Muchovej, S. J. ; Pérez, L. M. ; Pound, M. W. ; Teuben, P. J. ; Volgenau, N. H. ; Woody, D. P. ; Wright, M. C H ; Zauderer, B. A. / THE ionized circumstellar envelopes of orion source i and the becklin-neugebauer object. In: Astrophysical Journal. 2013 ; Vol. 765, No. 1.
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AU - Lamb, J. W.

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