Zobrazeno 1 - 10
of 136
pro vyhledávání: '"Plunkett, Adele"'
Autor:
Santamaria-Miranda, Alejandro, de Gregorio-Monsalvo, Itziar, Ohashi, Nagayoshi, Tobin, John J., Sai, Jinshi, Jorgensen, Jes K., Aso, Yusuke, Lin, Zhe-Yu Daniel, Flores, Christian, Kido, Miyu, Koch, Patrick M., Kwon, Woojin, Lee, Chang Won, Li, Zhi-Yun, Looney, Leslie W., Plunkett, Adele L., Takakuwa, Shigehisa, Hoff, Merel L. R van t, Williams, Jonathan P., Yen, Hsi-Wei
We present the results of the ALMA Large Program Early Planet Formation in Embedded disks observations of the Class 0 protostar GSS30 IRS3. Our observations included 1.3 mm continuum with a resolution of 0.''05 (7.8 au) and several molecular species
Externí odkaz:
http://arxiv.org/abs/2407.20885
Autor:
Gavino, Sacha, Jørgensen, Jes K., Sharma, Rajeeb, Yang, Yao-Lun, Li, Zhi-Yun, Tobin, John J., Ohashi, Nagayoshi, Takakuwa, Shigehisa, Plunkett, Adele, Kwon, Woojin, de Gregorio-Monsalvo, Itziar, Lin, Zhe-Yu Daniel, Santamaría-Miranda, Alejandro, Aso, Yusuke, Sai, Jinshi, Aikawa, Yuri, Tomida, Kengo, Koch, Patrick M., Lee, Jeong-Eun, Lee, Chang Won, Lai, Shih-Ping, Looney, Leslie W., Narayanan, Suchitra, Phuong, Nguyen Thi, Thieme, Travis J., Hoff, Merel L. R. van 't, Willians, Jonathan P., Yen, Hsi-Wei
We present Atacama Large Millimeter/submillimeter Array (ALMA) observations of the binary Class 0 protostellar system BHR 71 IRS1 and IRS2 as part of the Early Planet Formation in Embedded Disks (eDisk) ALMA Large Program. We describe the $^{12}$CO (
Externí odkaz:
http://arxiv.org/abs/2407.17249
Autor:
Assani, Korash, Harsono, Daniel, Ramsey, Jon, Li, Zhi-Yun, Bjerkeli, Per, Pontoppidan, Klaus, Tychoniec, Łukasz, Calcutt, Hannah, Kristensen, Lars, Jorgensen, Jes, Plunkett, Adele, van Gelder, Martijn, Francis, Logan
Publikováno v:
A&A 688, A26 (2024)
(abridged) Protostellar outflows exhibit large variations in their structure depending on the observed gas emission. This study analyzes the atomic jet and molecular outflow in the Class I protostar, TMC1A to characterize morphology and identify prev
Externí odkaz:
http://arxiv.org/abs/2404.18334
Autor:
Encalada, Frankie J., Looney, Leslie W., Takakuwa, Shigehisa, Tobin, John J., Ohashi, Nagayoshi, Jørgensen, Jes K., Li, Zhi-Yun, Aikawa, Yuri, Aso, Yusuke, Koch, Patrick M., Kwon, Woojin, Lai, Shih-Ping, Lee, Chang Won, Lin, Zhe-Yu Daniel, Santamarıa-Miranda, Alejandro, de Gregorio-Monsalvo, Itziar, Phuong, Nguyen Thi, Plunkett, Adele, Sai, Jinshi, Sharma, Rajeeb, Yen, Hsi-Wei, Han, Ilseung
Young protostellar binary systems, with expected ages less than $\sim$10$^5$ years, are little modified since birth, providing key clues to binary formation and evolution. We present a first look at the young, Class 0 binary protostellar system R CrA
Externí odkaz:
http://arxiv.org/abs/2403.14143
Molecular abundances in protoplanetary disks are highly sensitive to the local physical conditions, including gas temperature, gas density, radiation field, and dust properties. Often multiple factors are intertwined, impacting the abundances of both
Externí odkaz:
http://arxiv.org/abs/2312.05254
Autor:
Flores, Christian, Ohashi, Nagayoshi, Tobin, John J., Jørgensen, Jes K., Takakuwa, Shigehisa, Li, Zhi-Yun, Lin, Zhe-Yu Daniel, Hoff, Merel L. R. van 't, Plunkett, Adele L., Yamato, Yoshihide, Sai, Jinshi, Koch, Patrick M., Yen, Hsi-Wei, Aikawa, Yuri, Aso, Yusuke, de Gregorio-Monsalvo, Itziar, Kido, Miyu, Kwon, Woojin, Lee, Jeong-Eun, Lee, Chang Won, Looney, Leslie W., Santamaría-Miranda, Alejandro, Sharma, Rajeeb, Thieme, Travis J., Williams, Jonathan P., Han, Ilseung, Narayanan, Suchitra, Lai, Shih-Ping
We present ALMA observations of the Class I source Oph IRS63 in the context of the Early Planet Formation in Embedded Disks (eDisk) large program. Our ALMA observations of Oph IRS63 show a myriad of protostellar features, such as a shell-like bipolar
Externí odkaz:
http://arxiv.org/abs/2310.14617
Autor:
Narayanan, Suchitra, Williams, Jonathan P., Tobin, John J., Jorgensen, Jes K., Ohashi, Nagayoshi, Lin, Zhe-Yu Daniel, Hoff, Merel L. R. van't, Li, Zhi-Yun, Plunkett, Adele L., Looney, Leslie W., Takakuwa, Shigehisa, Yen, Hsi-Wei, Aso, Yusuke, Flores, Christian, Lee, Jeong-Eun, Lai, Shih-Ping, Kwon, Woojin, de Gregorio-Monsalvo, Itziar, Sharma, Rajeeb, Lee, Chang Won
We present the first results from the Early Planet Formation in Embedded Disks (eDisk) ALMA Large Program toward Oph IRS43, a binary system of solar mass protostars. The 1.3 mm dust continuum observations resolve a compact disk, ~6au radius, around t
Externí odkaz:
http://arxiv.org/abs/2310.15491
Autor:
Thieme, Travis J., Lai, Shih-Ping, Ohashi, Nagayoshi, Tobin, John J., Jørgensen, Jes K., Sai, Jinshi, Aso, Yusuke, Williams, Jonathan P., Yamato, Yoshihide, Aikawa, Yuri, de Gregorio-Monsalvo, Itziar, Han, Ilseung, Kwon, Woojin, Lee, Chang Won, Lee, Jeong-Eun, Li, Zhi-Yun, Lin, Zhe-Yu Daniel, Looney, Leslie W., Narayanan, Suchitra, Phuong, Nguyen Thi, Plunkett, Adele L., Santamaría-Miranda, Alejandro, Sharma, Rajeeb, Takakuwa, Shigehisa, Yen, Hsi-Wei
Protostellar disks are a ubiquitous part of the star formation process and the future sites of planet formation. As part of the Early Planet Formation in Embedded Disks (eDisk) large program, we present high-angular resolution dust continuum ($\sim40
Externí odkaz:
http://arxiv.org/abs/2310.12453
Autor:
Kido, Miyu, Takakuwa, Shigehisa, Saigo, Kazuya, Ohashi, Nagayoshi, Tobin, John J., K, Jes, Jørgensen, Aikawa, Yuri, Aso, Yusuke, Encalada, Frankie J., Flores, Christian, Gavino, Sacha, de Gregorio-Monsalvo, Itziar, Han, Ilseung, Hirano, Shingo, Koch, Patrick M., Kwon, Woojin, Lai, Shih-Ping, Lee, Chang Won, Lee, Jeong-Eun, Li, Zhi-Yun, Lin, Zhe-Yu Daniel, Looney, Leslie W., Mori, Shoji, Narayanan, Suchitra, Plunkett, Adele L., Phuong, Nguyen Thi, Sai, Jinshi, Santamarîa-Miranda, Alejandro, Sharma, Rajeeb, Sheehan, Patrick, Thieme, Travis J., Tomida, Kengo, Hoff, Merel L. R. van't, Williams, Jonathan P., Yamato, Yoshihide, Yen, Hsi-Wei
We present observations of the Class 0 protostar IRAS 16544-1604 in CB 68 from the ''Early Planet Formation in Embedded Disks (eDisk)'' ALMA Large program. The ALMA observations target continuum and lines at 1.3-mm with an angular resolution of $\sim
Externí odkaz:
http://arxiv.org/abs/2306.15443
Autor:
Hoff, Merel L. R. van 't, Tobin, John J., Li, Zhi-Yun, Ohashi, Nagayoshi, Jørgensen, Jes K., Lin, Zhe-Yu Daniel, Aikawa, Yuri, Aso, Yusuke, de Gregorio-Monsalvo, Itziar, Gavino, Sacha, Han, Ilseung, Koch, Patrick M., Kwon, Woojin, Lee, Chang Won, Lee, Jeong-Eun, Looney, Leslie W., Narayanan, Suchitra, Plunkett, Adele, Sai, Jinshi, Santamaría-Miranda, Alejandro, Sharma, Rajeeb, Sheehan, Patrick D., Takakuwa, Shigehisa, Thieme, Travis J., Williams, Jonathan P., Lai, Shih-Ping, Phuong, Nguyen Thi, Yen, Hsi-Wei
Studying the physical and chemical conditions of young embedded disks is crucial to constrain the initial conditions for planet formation. Here, we present Atacama Large Millimeter/submillimeter Array (ALMA) observations of dust continuum at $\sim$0.
Externí odkaz:
http://arxiv.org/abs/2306.15407