The Herschel first look at protostars in the Aquila rift

S. Bontemps; Ph. André; V. K?nyves; A. Menshchikov; N. Schneider; A. Maury; N. Peretto; D. Arzoumanian; M. Attard; F. Motte; V. Minier; P. Didelon; P. Saraceno; A. Abergel; J.-P. Baluteau; J.-Ph. Bernard; L. Cambrésy; P. Cox; J. Di Francesco; A. M. Di Giorgo; M. Griffin; P. Hargrave; M. Huang; J. Kirk; J. Li; P. Martin; B. Merín; S. Molinari; G. Olofsson; S. Pezzuto; T. Prusti; H. Roussel; D. Russeil; M. Sauvage; B. Sibthorpe; L. Spinoglio; L. Testi; R. Vavrek; D. Ward-Thompson; G. White; C. Wilson; A. Woodcraft; A. Zavagno

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The Herschel first look at protostars in the Aquila rift

机译：赫歇尔首先看了天鹰座裂谷中的原星

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As part of the science demonstration phase of the Herschel mission of the Gould Belt key program, the Aquila rift molecular complex has been observed. The complete imaging with SPIRE 250/350/500m and PACS 70/160mallows a deep investigation of embedded protostellar phases, probing ofthe dust emission from warm inner regions at 70 and 160m to the bulk of the cold envelopes between 250 and 500m. We used a systematic detection technique operating simultaneously on all Herschelbands to build a sample of protostars. Spectral energy distributionsare derived to measure luminosities and envelope masses, and to placethe protostars in an evolutionary diagram. The spatial distribution of protostars indicatesthree star-forming sites in Aquila, with W40/Sh2-64 H II region by farthe richest. Most of the detected protostars are newly discovered. Fora reduced area around the Serpens South cluster, we could compare the Herschel census of protostars with Spitzer results. The Herschel protostars are younger than in Spitzer with 7 Class0 YSOs newly revealed by Herschel. For the entire Aquila field, we find a total of 45-60 Class0YSOs discovered by Herschel. This confirms the global statistics of several hundred Class0 YSOs that should be found in the whole Gould Belt Survey.Key words: stars: formation - ISM: clouds

机译：作为古尔德带（Gould Belt）关键计划的赫歇尔（Herschel）任务的科学演示阶段的一部分，已观测到天鹰座裂谷分子复合物。使用SPIRE 250/350 / 500m和PACS 70/160进行的完整成像可以对埋藏的原星阶段进行深入研究，探测从70和160m温暖的内部区域到250至500m之间的大部分冷包层的尘埃排放。我们使用了一种系统的检测技术，该技术在所有Herschelband上同时运行，以构建原恒星样本。得出光谱能量分布以测量光度和包络质量，并将原恒星置于演化图中。原恒星的空间分布表明，天鹰座有3个恒星形成地点，其中W40 / Sh2-64 H II区域最丰富。大多数检测到的原恒星都是新发现的。对于Serpens South星团周围的缩小区域，我们可以将原星的赫歇尔普查与Spitzer结果进行比较。 Herschel的原星比Spitzer的年轻，Herschel新揭示了7种Class0 YSO。对于整个Aquila领域，我们发现Herschel共发现了45至60个Class0YSO。这证实了在整个古尔德带调查中应该发现的数百种Class0 YSO的全球统计数据。关键词：恒星：编队-ISM：云

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《Astronomy and astrophysics》 |2010年第19期|共5页
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S. Bontemps; Ph. André; V. K?nyves; A. Menshchikov; N. Schneider; A. Maury; N. Peretto; D. Arzoumanian; M. Attard; F. Motte; V. Minier; P. Didelon; P. Saraceno; A. Abergel; J.-P. Baluteau; J.-Ph. Bernard; L. Cambrésy; P. Cox; J. Di Francesco; A. M. Di Giorgo; M. Griffin; P. Hargrave; M. Huang; J. Kirk; J. Li; P. Martin; B. Merín; S. Molinari; G. Olofsson; S. Pezzuto; T. Prusti; H. Roussel; D. Russeil; M. Sauvage; B. Sibthorpe; L. Spinoglio; L. Testi; R. Vavrek; D. Ward-Thompson; G. White; C. Wilson; A. Woodcraft; A. Zavagno;
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1. The Herschel first look at protostars in the Aquila rift [J] . S. Bontemps, Ph. André, V. K?nyves, Astronomy and astrophysics . 2010,第20期

机译：赫歇尔首先看了天鹰座裂谷中的原星
2. CO in Protostars (COPS): Herschel-SPIRE Spectroscopy of Embedded Protostars* [J] . Yao-Lun Yang, Joel D. Green, Neal J. Evans II, The Astrophysical journal . 2018,第2期

机译：Protostars（COPS）中的CO：嵌入式Protostars的Herschel-SPIRE光谱*
3. Multi-line Herschel/HIFI observations of water reveal infall motions and chemical segregation around high-mass protostars ★ ★★ [J] . F. F. S. van der Tak, R. F. Shipman, T. Jacq, Astronomy and astrophysics . 2019,第19期

机译：对水的多行 Herschel / HIFI观测揭示了高质量原恒星周围的坠落运动和化学偏析★ ★★
4. A SUBMILLIMETER LINE SURVEY OF LOW-MASS PROTOSTARS: PRELUDE TO ALMA AND HERSCHEL [C] . E.F. van Dishoeck, J.K. Jorgensen, S. Maret, Conference on The Dusty and Molecular Universe: A Prelude to Herschel and ALMA . 2005

机译：低质量矩阵的亚颌胶线调查：对Alma和Herschel的前奏
5. Lithospheric Controls on the Rifting of the Tanzanian Craton at the Eyasi Rift, Eastern Branch of the East African Rift System [D] . Fletcher, Andrew W. 2017

机译：东非裂谷系统东部分支Eyasi裂谷对坦桑尼亚克拉通裂谷的岩石圈控制
6. Optical polarization and infrared spectrum of a possible protostar in a reflection nebula [O] . E. P. Ney, B. F. Hatfield, R. D. Gehrz 1980

机译：反射星云中可能存在的原恒星的光学偏振和红外光谱
7. The Herschel first look at protostars in the Aquila rift [Letter] [O] . Bontemps, S., André, Ph., Könyves, V., 2010

机译：赫歇尔首先看了天鹰座裂谷中的原恒星[字母]
8. HERschel Inventory of the Agents of Galaxy Evolution in the Magellanic Clouds, a HERschel Open Time Key Program. [R] . Meixner, M., Panuzzo, P., Misselt, K., 2013

机译：HERschel麦哲伦星云中星系演化特征库存，HERschel开放时间关键程序。

The Herschel first look at protostars in the Aquila rift

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