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Items where Person is "Zavagno-A"

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Zhang, S. and Zavagno, A. and Yuan, J. et al. (2020) H II regions and high-mass starless clump candidates. I. Catalogs and properties. Astronomy and Astrophysics, 637 . Art. No. A40. ISSN 0004-6361.


Montillaud, J. and Juvela, M. and Rivera-Ingraham, A. et al. (2015) Galactic cold cores. IV. Cold submillimetre sources: catalogue and statistical analysis. Astronomy and Astrophysics, 584 . Art. No. A92. ISSN 0004-6361.


Juvela, M. and Ristorcelli, I. and Pagani, L. et al. (2012) Galactic cold cores. III. General cloud properties. Astronomy and Astrophysics, 541 . Art. No. A12. ISSN 0004-6361.

Anderson, L. D. and Zavagno, A. and Barlow, M. J. et al. (2012) Distinguishing between HII regions and planetary nebulae with Hi-GAL, WISE, MIPSGAL, and GLIMPSE. Astronomy and Astrophysics, 537 . Art. No. A1. ISSN 0004-6361.


Juvela, M. and Ristorcelli, I. and Pelkonen, V.-M. et al. (2011) Galactic cold cores. II. Herschel study of the extended dust emission around the first Planck detections. Astronomy and Astrophysics, 527 . Art. No. A111. ISSN 0004-6361.

Russeil, D. and Pestalozzi, M. and Mottram, J. C. et al. (2011) Giving physical significance to the Hi-GAL data: determining the distance of cold dusty cores in the Milky Way. Astronomy and Astrophysics, 526 . Art. No. A151. ISSN 0004-6361.


Kirk, J. M. and Polehampton, E. and Anderson, L. D. et al. (2010) Herschel-SPIRE spectroscopy of G29.96-0.02: Fitting the full SED. Astronomy and Astrophysics, 518 . Art. No. L82. ISSN 0004-6361.

Zavagno, A. and Anderson, L. D. and Russeil, D. et al. (2010) Star formation triggered by H II regions in our Galaxy: First results for N49 from the Herschel infrared survey of the Galactic plane. Astronomy and Astrophysics, 518 . L101. ISSN 0004-6361.

Molinari, S. and Swinyard, B. and Bally, J. et al. (2010) Hi-GAL: The Herschel Infrared Galactic Plane Survey. Publications of the Astronomical Society of the Pacific, 122 (889). pp. 314-325. ISSN 0004-6280.

This list was generated on Fri Dec 4 13:41:07 2020 PST.