Access the full text.
Sign up today, get DeepDyve free for 14 days.
S. Bergh (1975)
DISCOVERY OF HERBIG-HARO OBJECTS BY [S II] INTERFERENCE PHOTOGRAPHYPublications of the Astronomical Society of the Pacific, 87
T. Sitnik, A. Rastorguev, A. Tatarnikova, A. Tatarnikov, O. Egorov, A. Tatarnikov (2020)
A revision of the vdB 130 cluster stellar content based on Gaia DR2 data: interstellar extinction toward the Cyg OB1 supershellMonthly Notices of the Royal Astronomical Society, 498
Shu Wang, Xiaodian Chen (2019)
The Optical to Mid-infrared Extinction Law Based on the APOGEE, Gaia DR2, Pan-STARRS1, SDSS, APASS, 2MASS, and WISE SurveysThe Astrophysical Journal, 877
K Dobashi (2011)
10.1093/pasj/63.sp1.S1Publ. Astron. Soc. Japan, 63
SN Dodonov (2017)
10.1134/S1990341317040113Astrophys. Bull., 72
F Anders (2022)
10.1051/0004-6361/202142369Astron. Astrophys., 658
(1975)
A . L . Gyul ’ budagyan , R . Shvarts , and F . S . Nazaretyan , Soobshch
C. Bailer-Jones, J. Rybizki, M. Fouesneau, M. Demleitner, R. Astronomy, Heidelberg, A. Rechen-Institut (2020)
Estimating distances from parallaxes. V: Geometric and photogeometric distances to 1.47 billion stars in Gaia Early Data Release 3.arXiv: Solar and Stellar Astrophysics
F. Anders, A. Khalatyan, C. Chiappini, A. Queiroz, B. Santiago, C. Jordi, L. Girardi, A. Brown, G. Matijevič, G. Monari, T. Cantat-Gaudin, M. Weiler, Saniya Khan, A. Miglio, I. Carrillo, M. Romero-Gómez, I. Minchev, R. Jong, T. Antoja, P. Ramos, M. Steinmetz, H. Enke (2019)
Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18Astronomy & Astrophysics
D. Froebrich, A. Scholz, C. Raftery, Dublin Studies, 2. Dublin, Ireland Toronto, Toronto, Canada. Dublin, Ireland Astrophysics, S. Science, U. Kent, Canterbury, UK. (2006)
A systematic survey for infrared star clusters with |b| < 20° using 2MASSMonthly Notices of the Royal Astronomical Society, 374
T. Movsessian, T. Magakian, S. Observatory, Armenia, S. Observatory, Russia. (2020)
New Herbig–Haro objects and outflows in the Mon R1 associationarXiv: Solar and Stellar Astrophysics
R. Scholz, N. Kharchenko, A. Piskunov, A. Piskunov, S. Röser, E. Schilbach, E. Schilbach (2015)
Global survey of star clusters in the Milky Way - IV. 63 new open clusters detected by proper motionsAstronomy and Astrophysics, 581
CAL Bailer-Jones (2021)
10.3847/1538-3881/abd806Astron. J., 161
T. Movsessian, T. Magakian, H. Andreasyan (2022)
HH 1216: The Extended Bipolar Flow Associated with IRAS 06212-1049Astrophysics, 65
N. Kharchenko, A. Piskunov, A. Piskunov, E. Schilbach, S. Röser, R. Scholz (2013)
Global survey of star clusters in the Milky Way II. The catalogue of basic parametersAstronomy and Astrophysics, 558
NV Kharchenko (2013)
10.1051/0004-6361/201527292Astron. Astrophys., 585
Two new Herbig-Haro flows were found in a study of the isolated Dobashi 5006 dark cloud (l = 216°.7, b = –13°.9): one certain (HH 1179) and one presumable, associated with the infrared sources 2MASS 06082284-0936139 and 2MASS 06081525-0933490, correspondingly. Judging from their spectral energy distributions, these sources may be Class 1 objects with luminosities of order 23 L⨀ and 3.6 L⨀, respectively. They are part of the poor star cluster MWSC 0739, study of which based on data from the Gaia DR3 survey has made it possible to detect 17 stars which are probably members of it. A list of them and their main parameters is given. The distance of the cluster is estimated to be 820 pc and the color excess on the path to the cluster is E(BP - RP) ≈ 1.05 mag. All of these stars are PMS-objects and most of them are optically variable. It is concluded that the newly discovered compact star-formation zone in the Dobashi 5006 cloud has an age of no more than a few million years and this process continues up to the present time.
Astrophysics – Springer Journals
Published: Mar 1, 2023
Keywords: Herbig-Haro objects; young stars; Dobashi 5006
Read and print from thousands of top scholarly journals.
Already have an account? Log in
Bookmark this article. You can see your Bookmarks on your DeepDyve Library.
To save an article, log in first, or sign up for a DeepDyve account if you don’t already have one.
Copy and paste the desired citation format or use the link below to download a file formatted for EndNote
Access the full text.
Sign up today, get DeepDyve free for 14 days.
All DeepDyve websites use cookies to improve your online experience. They were placed on your computer when you launched this website. You can change your cookie settings through your browser.