Molecular Hydrogen Emission from Cold Condensations in NGC 2440
نویسندگان
چکیده
منابع مشابه
Near - IR Fluorescent Molecular Hydrogen Emission from NGC 2023
Spectra from 1 to 2 ·5 μm, at 230–430 spectral resolution, are presented of the fluorescent molecular hydrogen line emission from two locations in the reflection nebula NGC 2023. Over 100 H2 lines can be identified in the spectra, although blending and poor atmospheric transmission mean that reliable level column densities can only be obtained from 35 lines. This latter group includes lines fro...
متن کاملNear - Infrared Spectroscopy of Molecular Hydrogen Emission in Four Reflection Nebulae : NGC 1333 , NGC 2023 , NGC 2068 , and NGC 7023
We present near-infrared spectroscopy of fluorescent molecular hydrogen (H2) emission from NGC 1333, NGC 2023, NGC 2068, and NGC 7023 and derive the physical properties of the molecular material in these reflection nebulae. Our observations of NGC 2023 and NGC 7023 and the physical parameters we derive for these nebulae are in good agreement with previous studies. Both NGC 1333 and NGC 2068 hav...
متن کاملTrapping cold molecular hydrogen.
Translationally cold H(2) molecules excited to non-penetrating |M(J)| = 3 Rydberg states of principal quantum number in the range 21-37 have been decelerated and trapped using time-dependent inhomogeneous electric fields. The |M(J)| = 3 Rydberg states were prepared from the X (1)Σ(+)(u)(v = 0, J = 0) ground state using a resonant three-photon excitation sequence via the B (1)Σ(+)(u)(v = 3, J = ...
متن کاملMolecular hydrogen emission from protoplanetary disks
We have modeled self-consistently the density and temperature profiles of gas and dust in protoplanetary disks, taking into account irradiation from a central star. Making use of this physical structure, we have calculated the level populations of molecular hydrogen and the line emission from the disks. As a result, we can reproduce the observed strong line spectra of molecular hydrogen from pr...
متن کاملMolecular Hydrogen emission from disks in the eta Chamaeleontis cluster
Disks in the 6 Myr old cluster η Chamaeleontis were searched for emission from hot H2 . Around the M3 star ECHA J0843.4-7905 we detect circumstellar gas orbiting at ∼2 AU. If the gas is UV-excited, the ro-vibrational line traces a hot gas layer supported by a disk of mass ∼0.03 M⊙ , similar to the minimum mass solar nebula. Such a gas reservoir at 6 Myr would promote the formation and inwards m...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Symposium - International Astronomical Union
سال: 1989
ISSN: 0074-1809
DOI: 10.1017/s0074180900138185