2026ApJ...997..239B


Query : 2026ApJ...997..239B

2026ApJ...997..239B - Astrophys. J., 997, 239 (2026/February-1)

SPHEREx: Aromatics, Aliphatics, and PAH Size across the Iris Nebula.

BOERSMA C., MARAGKOUDAKIS A., ALLAMANDOLA L.J., BREGMAN J.D., TEMI P., ESPOSITO V.J. and FORTENBERRY R.C.

Abstract (from CDS):

Observations by the Spectro-Photometer for the History of the Universe, Epoch of Reionization, and Ices Explorer (SPHEREx) are combined with counterpart Spitzer spectral map data to study the aromatic, aliphatic, and polycyclic aromatic hydrocarbon (PAH) size evolution across the northwest photodissociation region (PDR) of the Iris Nebula (NGC 7023). The 3.3-3.4 μm complex (I3.3) and 11.2 μm (I11.2) PAH band strength are determined through direct integration. In addition, the former is decomposed into a 3.3 (${\rm{I}}{{\prime} }_{3.3}$) and 3.4 μm (${\rm{I}}{{\prime} }_{3.4}$) subfeature by fitting SPHEREx bandpass-integrated photometry using a modeled, highly sampled, multicomponent spectrum. I3.3, I11.2, ${\rm{I}}{{\prime} }_{3.3}$, and ${\rm{I}}{{\prime} }_{3.4}$ all peak at the PDR. The NASA Ames PAH IR Spectroscopic Database is used to obtain the average number of carbon atoms ($\bar{{N}_{{\rm{C}}}}$) and small PAH fraction (fsmall) by fitting the isolated PAH component of the Spitzer segment: $70\lesssim \bar{{N}_{{\rm{C}}}}\lesssim 76$ and 0.24 ≲ fsmall ≲ 0.36, respectively. ${\rm{I}}{{\prime} }_{3.4}$/${\rm{I}}{{\prime} }_{3.3}$, I11.2/I3.3, $\bar{{N}_{{\rm{C}}}}$, and fsmall all show a demarcation that matches the large-scale morphology of the region. For ${\rm{I}}{{\prime} }_{3.3}$ and ${\rm{I}}{{\prime} }_{3.4}$ this is reflected by two distinct trends when plotted against each other, one associated with the dense medium and the other with the diffuse medium: ${[{N}_{{\rm{H}},{\rm{ali}}}/{N}_{{\rm{H}},{\rm{aro}}}]}_{{\rm{dense}}}$ = 0.42 ± 0.01 and ${[{N}_{{\rm{H}},{\rm{ali}}}/{N}_{{\rm{H}},{\rm{aro}}}]}_{{\rm{diffuse}}}$ = 0.10 ± 0.01, respectively. $\bar{{N}_{{\rm{C}}}}$ and fsmall are tentatively correlated with I11.2/I3.3 (R = 0.54 ± 0.05 and -0.45 ± 0.05, respectively). A wider variety of large(r) extended interstellar medium objects is required to tighten the correlations, turn them into quantitative calibrators for PAH size, and pin down the discrepancy of correlations with ${\rm{I}}{{\prime} }_{3.3}$ involved.

Abstract Copyright: © 2026. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Polycyclic aromatic hydrocarbons - Near infrared astronomy - Interstellar molecules - Laboratory astrophysics - Reflection nebulae

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME Orion Bright Bar reg 05 35 22.30 -05 24 33.0           ~ 1004 0
2 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 16269 0
3 NGC 7023 OpC 21 01 36.9 +68 09 48           ~ 739 0
4 HD 200775 Ae* 21 01 36.9205762896 +68 09 47.789578836 7.34 7.754 7.427 8.13   B2Ve 582 0

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