On the Nature of the Enigmatic Object IRAS 19312+1950: A Rare Phase of Massive Star Formation?
Artikel i vetenskaplig tidskrift, 2016

IRAS 19312+1950 is a peculiar object that has eluded firm characterization since its discovery, with combined maser properties similar to an evolved star and a young stellar object (YSO). To help determine its true nature, we obtained infrared spectra of IRAS 19312+1950 in the range 5–550 μm using the Herschel and Spitzer space observatories. The Herschel PACS maps exhibit a compact, slightly asymmetric continuum source at 170 μm, indicative of a large, dusty circumstellar envelope. The far-IR CO emission line spectrum reveals two gas temperature components: ≈0.22 solar masses of material at 280 ± 18 K, and ≈1.6 solar masses of material at 157 ± 3 K. The O i 63 μm line is detected on-source but no significant emission from atomic ions was found. The HIFI observations display shocked, high-velocity gas with outflow speeds up to 90 km/s along the line of sight. From Spitzer spectroscopy, we identify ice absorption bands due to H2O at 5.8 μm and CO2 at 15 μm. The spectral energy distribution is consistent with a massive, luminous (~2 × 10^4 solar luminosities) central source surrounded by a dense, warm circumstellar disk and envelope of total mass ~500–700 solar masses, with large bipolar outflow cavities. The combination of distinctive far-IR spectral features suggest that IRAS 19312+1950 should be classified as an accreting, high-mass YSO rather than an evolved star. In light of this reclassification, IRAS 19312+1950 becomes only the fifth high-mass protostar known to exhibit SiO maser activity, and demonstrates that 18 cm OH maser line ratios may not be reliable observational discriminators between evolved stars and YSOs.

stars: formation


ISM: molecules

stars: winds


stars: protostars

stars: AGB and post-AGB


M. A. Cordiner

NASA Goddard Space Flight Center

Catholic University of America

A. Boogert

Universities Space Research Association

S.B. Charnley

NASA Goddard Space Flight Center

Kay Justtanont

Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik

N. L. J. Cox

KU Leuven

Universite de Toulouse

R. G. Smith

University of New South Wales (UNSW) Australia

Aggm Tielens

Leiden Observatory Research Institute

Eva Wirström

Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik

S. N. Milam

NASA Goddard Space Flight Center

J. V. Keane

University of Hawaii at Manoa

Astrophysical Journal

0004-637X (ISSN) 1538-4357 (eISSN)

Vol. 828 51


Astronomi, astrofysik och kosmologi


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