Zobrazeno 1 - 10
of 52
pro vyhledávání: '"Aditya Dayal"'
Autor:
Tyagi, Aditya Dayal, Asawa, Krishna
Publikováno v:
International Journal of Performability Engineering; Sep2024, Vol. 20 Issue 9, p552-562, 11p
Publikováno v:
International Journal of Advanced Research in Science, Communication and Technology. :316-325
The human face is a crucial organ for conveying an individual's emotional state and behavior. However, manually creating a playlist based on an individual's emotional features can be a labor-intensive and time-consuming task. To automate this process
Autor:
Joseph L. Hora, Giovanni G. Fazio, T. M. Bania, Dan P. Clemens, Lynne K. Deutsch, Kathleen E. Kraemer, James M. Jackson, Robert Simon, Mark H. Heyer, Aditya Dayal, Marc Kassis, William F. Hoffmann
Publikováno v:
The Astrophysical Journal. 588:918-930
We have imaged five dense molecular cores, selected from the Galactic Ring Survey (GRS), in the mid-infrared with the MIRAC3 instrument. We obtained high spatial resolution (~1'') images through narrowband filters at 12.5 and 20.6 μm. Four of the fi
Autor:
James M. Jackson, Lynne K. Deutsch, Marc Kassis, William F. Hoffmann, Joseph L. Hora, Kathleen E. Kraemer, Aditya Dayal, Giovanni G. Fazio
Publikováno v:
The Astrophysical Journal. 561:282-298
Four massive star-forming regions were imaged in the mid-infrared with the MIRAC3 instrument: W51 IRS 2, Mon R2, DR 21, and S140. We obtained high spatial resolution (~1'') images at several wavelengths from 7.8 to 13.2 μm with the circular variable
Autor:
Aditya Dayal, Lynne K. Deutsch, Massimo Marengo, Giovanni G. Fazio, Margarita Karovska, Joseph L. Hora, William F. Hoffmann
Publikováno v:
The Astrophysical Journal. 556:L47-L50
This paper presents results from high-angular resolution mid-IR imaging of the Mira AB circumbinary environment using the MIRAC3 camera at the NASA Infrared Telescope Facility (IRTF). We resolved the dusty circumstellar envelope at 9.8, 11.7 and 18 m
Autor:
Giovanni G. Fazio, Lynne K. Deutsch, Toshiya Ueta, William F. Hoffmann, Aditya Dayal, Joseph L. Hora, Margaret Meixner
Publikováno v:
The Astrophysical Journal. 548:1020-1028
We report detection of an extended mid-infrared emission from \iras 18576+0341 (AFGL 2298). The object shows a dusty circumstellar shell that has diameter of $\age 7\arcsec$ at 10.3 and 18.0 $\um$. The dust nebula shows two emission peaks concentrica
Autor:
William F. Hoffmann, Lynne K. Deutsch, Massimo Marengo, Aditya Dayal, Joseph L. Hora, Ray Jayawardhana, Giovanni G. Fazio
Publikováno v:
The Astrophysical Journal. 541:L63-L66
Most, if not all, stars are now believed to produce energetic outflows during their formation. Yet, almost 20 years after the discovery of bipolar outflows from young stars, the origins of this violent phenomenon are not well understood. One of the d
Autor:
Alberto D. Bolatto, Kathleen E. Kraemer, Joseph L. Hora, Nathan Smith, James M. Jackson, William F. Hoffmann, Lynne K. Deutsch, Giovanni G. Fazio, Aditya Dayal
Publikováno v:
The Astrophysical Journal. 540:316-331
Several compact radio continuum sources in W49A show detectable 8-20 μm emission in MIRAC2 images obtained at the IRTF. In general, the infrared morphologies of these sources closely resemble the radio continuum emission. Spectral energy distributio
Autor:
John H. Bieging, William B. Latter, Douglas M. Kelly, Aditya Dayal, Joseph L. Hora, Casey Meakin, Alexander G. G. M. Tielens
Publikováno v:
The Astrophysical Journal. 539:783-797
We report results from a Hubble Space Telescope (HST) and Near-Infrared Camera and Multiobject Spectrometer (NICMOS) program to study the distribution of hot neutral (molecular hydrogen) and ionized circumstellar material in the young planetary nebul
Autor:
Aditya Dayal, C. A. Garland, William F. Hoffmann, Joseph L. Hora, M. F. Campbell, Lynne K. Deutsch, Giovanni G. Fazio
Publikováno v:
The Astrophysical Journal. 536:816-830
We present mid-infrared images of the ultracompact H II region complex G34.3+0.2 taken on the IRTF through a 1.8% circular variable filter wheel at 8.0, 9.7, 11.2, 12.8, and 13.2 μm and through a 6.8% filter at 20.6 μm. Infrared emission was detect