Results 71 to 80 of about 71,444 (299)

Early Planet Formation in Embedded Disks (eDisk). VIII. A Small Protostellar Disk around the Extremely Low Mass and Young Class 0 Protostar IRAS 15398–3359

The Astrophysical Journal, 2023
Protostellar disks are an ubiquitous part of the star formation process and the future sites of planet formation. As part of the Early Planet Formation in Embedded Disks large program, we present high angular resolution dust continuum (∼40 mas) and ...
Travis J. Thieme, Shih-Ping Lai, Nagayoshi Ohashi, John J. Tobin, Jes K. Jørgensen, Jinshi Sai (Insa Choi), Yusuke Aso, Jonathan P. Williams, Yoshihide Yamato, Yuri Aikawa, Itziar de Gregorio-Monsalvo, Ilseung Han, Woojin Kwon, Chang Won Lee, Jeong-Eun Lee, Zhi-Yun Li, Zhe-Yu Daniel Lin, Leslie W. Looney, Suchitra Narayanan, Nguyen Thi Phuong, Adele L. Plunkett, Alejandro Santamaría-Miranda, Rajeeb Sharma, Shigehisa Takakuwa, Hsi-Wei Yen   +24 more
doaj   +1 more source

Quasi‐Static to Supersonic Energy Absorption of Nanoarchitected Tubulanes and Schwarzites

Advanced Functional Materials, EarlyView.
Nanoarchitected energy‐absorptive Tubulanes exhibit record energy absorption under quasi‐static conditions and exceptional inelastic energy dissipation under 750 m s−1 ballistics impact, with high performance spanning strain rates of 12 orders of magnitude.
Peter Serles, Alianna Maguire, Thomas Butruille, Jet Lem, Shuo Yang, Pedro Guerra Demingos, Sahar Choukir, Michel Haché, Boran Kumral, Katherine Jia, Charles Jia, Yu Zou, Chandra Veer Singh, Carlos M. Portela, Jun Lou, Pulickel M. Ajayan, Tobin Filleter   +16 more
wiley   +1 more source

Bolocam Survey for 1.1 mm Dust Continuum Emission in the c2d Legacy Clouds. II. Ophiuchus

The Astrophysical Journal, 2006
We present a large-scale millimeter continuum map of the Ophiuchus molecular cloud. Nearly 11 square degrees, including all of the area in the cloud with visual extinction more than 3 magnitudes, was mapped at 1.1 mm with Bolocam on the Caltech Submillimeter Observatory (CSO).
Young, K. E., Enoch, M. L., Evans II, N. J., Glenn, J., Sargent, A., Huard, T., Aguirre, J., Golwala, S., Haig, D., Harvey, P., Laurent, G., Mauskopf, P., Sayers, J.   +12 more
openaire   +2 more sources

A Comparison of the Stellar, CO, and Dust-continuum Emission from Three Star-forming HUDF Galaxies at z ∼ 2

The Astrophysical Journal, 2020
Abstract We compare the extent of the dust, molecular gas, and stars in three star-forming galaxies, at z = 1.4, 1.6, and 2.7, selected from the Hubble Ultra Deep Field based on their bright carbon monoxide (CO) and dust-continuum emission as well as their large rest-frame optical sizes. The galaxies have high stellar masses,
Cox, Pierre, Kaasinen, Melanie, Walter, Fabian, Novak, Mladen, Neeleman, Marcel, Smail, Ian, Boogaard, Leindert, da Cunha, Elisabete, Weiss, Axel, Liu, Daizhong, Decarli, Roberto, Popping, Gergö, Diaz-Santos, Tanio, Cortés, Paulo, Aravena, Manuel, van Der Werf, Paul, Riechers, Dominik, Inami, Hanae, Hodge, Jacqueline A., Rix, Hans-Walter, Cunha, Elisabete Da, Werf, Paul van Der, Hodge, Jacqueline   +22 more
openaire   +6 more sources

Significant Gas-to-Dust Ratio Asymmetry and Variation in the Disk of HD 142527 and the Indication of Gas Depletion

, 2015
We investigate the dust and gas distribution in the disk around HD 142527 based on ALMA observations of dust continuum, 13CO(3-2), and C18O(3-2) emission.
Akiyama, Eiji, Fujiwara, Hideaki, Fukagawa, Misato, Hanawa, Tomoyuki, Honda, Mitsuhiko, Inutsuka, Shu-ichiro, Kataoka, Akimasa, Kitamura, Yoshimi, Kobayashi, Hiroshi, Momose, Munetake, Muto, Takayuki, Nomura, Hideko, Saigo, Kazuya, Shibai, Hiroshi, Takahashi, Sanemichi Z., Takeuchi, Taku, Tsukagoshi, Takashi   +16 more
core   +1 more source

Early Planet Formation in Embedded Disks (eDisk). XVII. A Compact but Structured Keplerian Disk and Large-scale Streamers Revealed in the Class I Protostellar System IRAS 04169+2702

The Astrophysical Journal
We present high-resolution (∼0 $\mathop{.}\limits^{^{\prime\prime} }$ 05; 8 au) dust continuum and molecular line observations toward the Class I protostellar system IRAS 04169+2702 in the Taurus B213 region, as part of the Atacama Large Millimeter ...
Ilseung Han, Woojin Kwon, Yusuke Aso, Nagayoshi Ohashi, John J. Tobin, Jes K. Jørgensen, Shigehisa Takakuwa, Leslie W. Looney, Yuri Aikawa, Christian Flores, Itziar de Gregorio-Monsalvo, Patrick M. Koch, Chang Won Lee, Jeong-Eun Lee, Zhi-Yun Li, Zhe-Yu Daniel Lin, Jinshi Sai, Travis J. Thieme, Jonathan P. Williams, Sacha Gavino, Miyu Kido, Shih-Ping Lai, Nguyen Thi Phuong, Alejandro Santamaría-Miranda, Hsi-Wei Yen   +24 more
doaj   +1 more source

Strain‐Programmable Luminescent Adhesive Patch With Tartrazine‐Mediated Optical Skin Clearing for Photochemical Tissue Bonding

Advanced Functional Materials, EarlyView.
We propose a suture‐complementary approach that integrates optical skin clearing with a strain‐programmable luminescent adhesive patch. Hyaluronic acid promotes transdermal delivery of tartrazine to improve optical clearing and stabilizes its interaction with a photosensitizer. Optical clearing increases the penetration depth of visible light into skin,
Seong‐Jong Kim, Kyungjoo Jo, Kwanghyeon Park, Jun Hee Kim, Jong Hyeong Cho, Inhoo Choi, Sei Kwang Hahn   +6 more
wiley   +1 more source

HIGH-RESOLUTION OBSERVATIONS OF DUST CONTINUUM EMISSION AT 340 GHz FROM THE LOW-MASS T TAURI STAR FN TAURI [PDF]

The Astrophysical Journal, 2010
FN Tau is a rare example of very low-mass T Tauri stars that exhibits a spatially resolved nebulosity in near-infrared scattering light. To directly derive the parameters of a circumstellar disk around FN Tau, observations of dust continuum emission at 340 GHz are carried out with the Submillimeter Array (SMA).
Momose, Munetake, Ohashi, Nagayoshi, Kudo, Tomoyuki, Tamura, Motohide, Kitamura, Yoshimi   +4 more
openaire   +2 more sources

Dust processing in photodissociation regions - Mid-IR emission modelling

, 2008
Mid-infrared spectroscopy of dense illuminated ridges (or photodissociation regions, PDRs) suggests dust evolution. Such evolution must be reflected in the gas physical properties through processes like photo-electric heating or H_2 formation.
A. Abergel, Abergel, Abergel, Abergel, Abergel, Allers, Anthony-Twarog, Arendt, Barnard, Berné, Bohlin, Boulanger, Boulanger, Boulanger, Burgh, Cardelli, Castor, Cesarsky, Clayton, Compiègne, Dartois, Dartois, Draine, Draine, Draine, Draine, Désert, E. Habart, Field, Fitzpatrick, Fitzpatrick, Fitzpatrick, Flagey, Freyer, Gatley, Giard, Goicoechea, Habart, Habart, Habart, Habing, Henyey, Hily-Blant, Hollenbach, Houck, Joblin, Johnstone, Jones, Jones, Jones, Kelsall, Kim, L. Verstraete, Laor, Laureijs, Li, M. Compiègne, Mathis, Mathis, Mathis, Miville-Deschênes, Pech, Peeters, Peeters, Perryman, Pety, Pety, Philipp, Pound, Rapacioli, Savage, Schaerer, Schiminovich, Schutte, Sellgren, Smith, Stepnik, Teyssier, Thronson, Verstraete, Verstraete, Ward-Thompson, Warren, Weingartner, Weingartner, Werner, Werner, Witt, Witt, Zubko   +89 more
core   +1 more source

Pushing the Atacama Large Millimeter/submillimeter Array to the Limit: 140 pc Resolution Observations of a z = 6.6 Quasar–Galaxy Merger Resolve Strikingly Different Morphologies of Dust Continuum and [C ii] 158 μm Emission

The Astrophysical Journal
We present $0\mathop{.}\limits^{^{\prime\prime} }026$ (140 pc) resolution Atacama Large Millimeter/submillimeter Array observations of [C ii ] 158 μ m and dust continuum emission of the z = 6.6 quasar J0305–3150, resolved over ∼​​​​​​300–400 independent ...
Romain A. Meyer, Bram Venemans, Marcel Neeleman, Roberto Decarli, Fabian Walter   +4 more
doaj   +1 more source